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Title: The Herschels and Modern Astronomy

Author: Agnes M. Clerke

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                Most recently updated: October 18, 2024

Language: English

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*** START OF THE PROJECT GUTENBERG EBOOK THE HERSCHELS AND MODERN ASTRONOMY ***

THE CENTURY SCIENCE SERIES.

      EDITED BY SIR HENRY E. ROSCOE, D.C.L., LL.D., F.R.S.


  THE HERSCHELS
  AND
  _MODERN ASTRONOMY_




The Century Science Series.

EDITED BY

SIR HENRY E. ROSCOE, D.C.L., F.R.S., M.P.


  =John Dalton and the Rise of Modern Chemistry.=
      By Sir HENRY E. ROSCOE, F.R.S.

  =Major Rennell, F.R.S., and the Rise of English Geography.=
      By CLEMENTS R. MARKHAM, C.B., F.R.S., President of the Royal
      Geographical Society.

  =The Herschels and Modern Astronomy.=
      By Miss AGNES M. CLERKE, Author of “A Popular History of
      Astronomy during the 19th Century,” &c.


  _In Preparation._

  =Justus von Liebig: his Life and Work.=
      By W. A. SHENSTONE, Science Master in Clifton College.

  =Michael Faraday: his Life and Work.=
      By Professor SILVANUS P. THOMPSON, F.R.S.

  =Clerk Maxwell and Modern Physics.=
      By R. T. GLAZEBROOK, F.R.S., Fellow of Trinity College,
      Cambridge.

  =Charles Lyell: his Life and Work.=
      By Rev. Professor T. G. BONNEY, F.R.S.

  =Humphry Davy.=
      By T. E. THORPE, F.R.S., Principal Chemist of the Government
      Laboratories.

  =Pasteur: his Life and Work.=
      By ARMAND RUFFER, Director of the British Institute of
      Preventive Medicine.

  =Charles Darwin and the Origin of Species.=
      By EDWARD B. POULTON, M.A., F.R.S., Hope Professor of Zoology
      in the University of Oxford.

  =Hermann von Helmholtz.=
      By A. W. RÜCKER, F.R.S., Professor of Physics in the Royal
      College of Science, London.


CASSELL & COMPANY, LIMITED, _London; Paris & Melbourne_.




[Illustration: SIR WILLIAM HERSCHEL.

_Ætat. 50._

(_From Abbott’s painting in the National Portrait Gallery._)]




  _THE CENTURY SCIENCE SERIES._

  THE HERSCHELS
  AND
  _MODERN ASTRONOMY_

  BY
  AGNES M. CLERKE

  AUTHOR OF
  “A POPULAR HISTORY OF ASTRONOMY DURING THE 19TH CENTURY,”
  “THE SYSTEM OF THE STARS,” ETC.


  CASSELL AND COMPANY, LIMITED
  _LONDON, PARIS & MELBOURNE_
  1895

  ALL RIGHTS RESERVED

[Illustration]




PREFACE.


The chief authority for the Life of Sir William Herschel is Mrs. John
Herschel’s “Memoir of Caroline Herschel” (London, 1876). It embodies
Caroline’s Journals and Recollections, the accuracy of which is
above suspicion. William himself, indeed, referred to her for dates
connected with his early life. The collateral sources of information
are few and meagre; they yield mere gleanings, yet gleanings worth
collecting. Professor E. S. Holden has had recourse to many of them
for his excellent little monograph entitled “Herschel, his Life and
Works” (London, 1881), which is usefully supplemented by “A Synopsis
of the Scientific Writings of Sir William Herschel,” prepared by the
same author with the aid of Professor Hastings. It made part of the
Smithsonian Report for 1880, and was printed separately at Washington
in 1881. But the wonderful series of papers it summarises have still
to be sought, one by one, by those desiring to study them effectually,
in the various volumes of the _Philosophical Transactions_ in which
they originally appeared. Their collection and republication is,
nevertheless, a recognised desideratum, and would fill a conspicuous
gap in scientific literature.

Sir John Herschel’s life has yet to be written. The published materials
for it are scanty, although they have been reinforced by the inclusion
in the late Mr. Graves’s “Life of Sir William Rowan Hamilton” (Dublin,
1882–9) of his correspondence with that remarkable man. The present
writer has, however, been favoured by the late Miss Herschel, and by
Sir William J. Herschel, with the perusal of a considerable number of
Sir John Herschel’s, as well as of Sir William’s, manuscript letters.
She also gratefully acknowledges the kind help afforded to her by Lady
Gordon and Miss Herschel in connection with the portraits reproduced
in this volume. For detailed bibliographical references, the articles
on Sir John, Sir William, and Caroline Herschel, in the “Dictionary of
National Biography,” may be consulted.




CONTENTS.


                                                                    PAGE
  CHAPTER
     I.--EARLY LIFE OF WILLIAM HERSCHEL                                9

    II.--THE KING’S ASTRONOMER                                        32

   III.--THE EXPLORER OF THE HEAVENS                                  53

    IV.--HERSCHEL’S SPECIAL INVESTIGATIONS                            75

     V.--THE INFLUENCE OF HERSCHEL’S CAREER ON MODERN ASTRONOMY       98

    VI.--CAROLINE HERSCHEL                                           115

   VII.--SIR JOHN HERSCHEL AT CAMBRIDGE AND SLOUGH                   142

  VIII.--EXPEDITION TO THE CAPE                                      162

    IX.--LIFE AT COLLINGWOOD                                         183

     X.--WRITINGS AND EXPERIMENTAL INVESTIGATIONS                    203




ILLUSTRATIONS.


                                                                    PAGE
  PORTRAIT OF SIR WILLIAM HERSCHEL                        _Frontispiece_

  PORTRAIT OF CAROLINE HERSCHEL                                      115

  PORTRAIT OF SIR JOHN HERSCHEL                                      142




THE HERSCHELS

AND

MODERN ASTRONOMY.




CHAPTER I.

EARLY LIFE OF WILLIAM HERSCHEL.


William Herschel was descended from one of three brothers, whose
Lutheran opinions made it expedient for them to quit Moravia early
in the seventeenth century. Hans Herschel thereupon settled as a
brewer at Pirna, in Saxony; his son Abraham rose to some repute as
a landscape-gardener in the royal service at Dresden; and Abraham’s
youngest son, Isaac, brought into the world with him, in 1707, an
irresistible instinct and aptitude for music. Having studied at Berlin,
he made his way in 1731 to Hanover, where he was immediately appointed
oboist in the band of the Hanoverian Guard. A year later he married
Anna Ilse Moritzen, by whom he had ten children. The fourth of these,
Frederick William, known to fame as _William_ Herschel, was born
November 15th, 1738.

His brilliant faculties quickly displayed themselves. At the
garrison-school he easily distanced his brother Jacob, his senior
by four years, and learned besides, privately, whatever French and
mathematics the master could teach him. He showed also a pronounced
talent for music, and was already, at fourteen, a proficient on the
hautboy and violin. In this direction lay his manifest destiny. His
father was now bandmaster of the Guard; he was poor, and had no other
provision to give his sons than to train them in his own art; and
thus William, driven by necessity to become self-supporting while
still a boy, entered the band as oboist in 1753. They were a family
of musicians. Of the six who reached maturity, only Mrs. Griesbach,
the elder daughter, gave no sign of personally owning a share in the
common gift, which descended, nevertheless, to her five sons, all noted
performers on sundry instruments.

William Herschel accompanied his regiment to England in 1755, with his
father and elder brother. He returned a year later, bringing with him
a copy of Locke “On the Human Understanding,” upon which he had spent
the whole of his small savings. Two of the three volumes thus acquired
were recovered by his sister after seventy years, and transmitted to
his son. The breaking-out of the Seven Years’ War proved decisive as to
his future life. Campaigning hardships visibly told upon his health;
his parents resolved, at all hazards, to rescue him from them; and
accordingly, after the disaster at Hastenbeck, July 26th, 1757, they
surreptitiously shipped him off to England. By this adventure, since he
was in the military service of the Elector of Hanover, George III. of
England, he incurred the penalties of desertion; but they were never
exacted, and were remitted by the King himself in 1782.

William Herschel was in his nineteenth year when he landed at Dover
with a French crown-piece in his pocket. Necessity or prudence kept
him for some time obscure; and we next hear of him as having played a
solo on the violin at one of Barbandt’s concerts in London, February
15th, 1760. In the same year he was engaged by the Earl of Darlington
to train the band of the Durham Militia, when his shining qualities
brought him to the front. The officers of the regiment looked with
astonishment on the phenomenal young German who had dropped among them
from some cloudy region; who spoke English perfectly, played like a
virtuoso, and possessed a curious stock of varied knowledge. Their
account of him at a mess-dinner excited the curiosity of Dr. Miller,
organist and historian of Doncaster, who, having heard him perform a
violin solo by Giardini, fell into a rapture, and invited him on the
spot to live with him.

He left nothing undone for the advancement of his _protégé_; procured
for him tuitions and leading concert engagements; and encouraged him,
in 1765, to compete for the post of organist at Halifax. Herschel’s
special qualifications were small; his chief rival, Dr. Wainwright, was
a skilled player, and at the trial performance evoked much applause
by his brilliant execution. Only the builder of the organ, an odd
old German named Schnetzler, showed dissatisfaction, exclaiming:
“He run about the keys like one cat; he gif my pipes no time for to
shpeak.” Then Herschel mounted the loft, and the church was filled
with a majestic volume of sound, under cover of which a stately melody
made itself heard. The “Old Hundredth” followed, with equal effect.
Schnetzler was beside himself with delight. “I vil luf dis man,” he
cried, “because he git my pipes time for to shpeak.” Herschel had
virtually provided himself with four hands. A pair of leaden weights
brought in his pocket served to keep down two keys an octave apart,
while he improvised a slow air to suit the continuous bass thus
mechanically supplied. The artifice secured him the victory.

This anecdote is certainly authentic. It is related by Dr. Miller from
personal knowledge. Nor is it inconsistent with a story told by Joah
Bates, of King’s College, Cambridge, a passionate lover of music.
Repairing to Halifax, his native place, to conduct the “Messiah” at
the opening of a new organ, he was accosted in the church by a young
man, who asked for an opportunity of practising on it. Although as yet,
he said, unacquainted with the instrument, he aspired to the place of
organist; and the absolute certitude of his manner so impressed Bates
that he not only granted his request, but became his warm patron.
The young man’s name was William Herschel. We hear, further, on Dr.
Burney’s authority, that he played first violin in Bates’s orchestra.

But the tide of his fortunes was flowing, and he knew how to “take it
at the flood.” Early in 1766 he removed to Bath as oboist in Linley’s
celebrated orchestra, which played daily in the Pump Room to enliven
the parade of blushing damsels and ruffling gallants pictured to our
fancy in Miss Austen’s novels. Bath was then what Beau Nash had made
it--the very focus of polite society. Turbans nodded over cards; gigs
threaded their way along Union Passage; Cheap Street was blocked with
vehicles; the Lower Rooms witnessed the nightly evolutions of the
country-dance; the Grove, as Doran reminds us, was brilliant with
beauty, coquelicot ribbons, smart pelisses, laced coats, and ninepins.
The feat of “tipping all nine for a guinea” was frequently performed;
and further excitement might be had by merely plucking some lampoons
from the trees, which seemed to bear them as their natural fruit.
Music, too, was in high vogue. The theatres were thronged; and Miss
Linley’s exquisite voice was still heard in the concert-halls.

On the 4th of October, 1767, the new Octagon Chapel was opened for
service, with Herschel as organist. How it was that he obtained this
“agreeable and lucrative situation” we are ignorant; but he had that
singular capacity for distinction which explains everything. The
Octagon Chapel became a centre of fashionable attraction, and he soon
found himself lifted on the wave of public favour. Pupils of high
rank thronged to him, and his lessons often mounted to thirty-five a
week. He composed anthems, psalm-tunes, even full services for his
assiduously-trained choir. His family were made sharers in his success.
He secured a post in Linley’s orchestra for his younger brother
Alexander, in 1771; and he himself fetched his sister Caroline to Bath
in 1772. Both were of very considerable help to him in his musical and
other enterprises, the latter of which gradually gained ground over the
former.

Music was never everything to William Herschel. He cultivated it with
ardour; composed with facility in the prevalent graceful Italian style;
possessed a keen appreciation and perfect taste. But a musical career,
however brilliant, did not satisfy him. The inner promptings of genius
told him to look beyond. The first thirty-five years of his life
were thus spent in diligently preparing to respond to an undeclared
vocation. Nothing diverted him from his purpose of self-improvement.
At first, he aimed chiefly at mastering the knowledge connected
with his profession. With a view to the theory of music, “I applied
myself early,” he said, in a slight autobiographical sketch sent to
Lichtenberg at Göttingen, “to all the branches of the mathematics,
algebra, conic sections, fluxions, etc. Contracting thereby an
insatiable desire for knowledge in general, I extended my application
to languages--French, Italian, Latin, English--and determined to devote
myself entirely to the pursuit of knowledge, in which I resolved to
place all my future enjoyment and felicity. This resolution I have
never had occasion to change.” At Bath, in the midst of engrossing
musical occupations, his zeal for study grew only the more intense.
After fourteen or sixteen hours of teaching, he would “unbend his mind”
by plunging into Maclaurin’s “Fluxions,” or retire to rest with a basin
of milk, Smith’s “Opticks,” and Ferguson’s “Astronomy.” He had no
sooner fallen under the spell of this last science than he “resolved to
take nothing upon trust, but to see with my own eyes all that other men
had seen before.”

He hired, to begin with, a small reflector; but what it showed him
merely whetted his curiosity. And the price of a considerably larger
instrument proved to be more than he could afford to pay. Whereupon
he took the momentous resolution of being, for the future, his own
optician. This was in 1772. He at first tried fitting lenses into
pasteboard tubes, with the poor results that can be imagined. Then he
bought from a Quaker, who had dabbled in that line, the discarded
rubbish of his tools, patterns, polishers, and abortive mirrors; and in
June, 1773, when fine folk had mostly deserted Bath for summer resorts,
work was begun in earnest. The house was turned topsy-turvy; the two
brothers attacked the novel enterprise with boyish glee. Alexander,
a born mechanician, set up a huge lathe in one of the bedrooms; a
cabinet-maker was installed in the drawing-room; Caroline, in spite of
secret dismay at such unruly proceedings, lent a hand, and kept meals
going; William directed, inspired, toiled, with the ardour of a man
who had staked his life on the issue. Meanwhile, music could not be
neglected. Practising and choir-training went on; novelties for the
ensuing season were prepared; compositions written, and parts copied.
Then the winter brought the usual round of tuitions and performances,
while all the time mirrors were being ground and polished, tried and
rejected, without intermission. At last, after _two hundred_ failures,
a tolerable reflecting telescope was produced, about five inches in
aperture, and of five and a half feet focal length. The outcome may
seem small for so great an expenditure of pains; but those two hundred
failures made the Octagon Chapel organist an expert, unapproached
and unapproachable, in the construction of specula. With his new
instrument, on March 4th, 1774, he observed the Nebula in Orion; and a
record of this beginning of his astronomical work is still preserved by
the Royal Society.

William Herschel was now, as to age, _in mezzo cammin_. He had numbered
just so many years as had Dante when he began the “Divina Commedia.”
But he had not, like Dante, been thrown off the rails of life. The
rush of a successful professional career was irresistibly carrying him
along. Almost any other man would have had all his faculties absorbed
in it. Herschel’s were only stimulated by the occupations which it
brought. Yet they were of a peculiarly absorbing nature. Music is
the most exclusive of arts. In turning aside, after half a lifetime
spent in its cultivation, to seek his ideal elsewhere, Herschel took
an unparalleled course. And his choice was final. Music was long his
pursuit, astronomy his pastime; a fortunate event enabled him to make
astronomy his pursuit, while keeping music for a pastime.

Yet each demands a totally different kind of training, not only of
the intellect, but of the senses. From his earliest childhood William
Herschel’s nerves and brain had been specially educated to discriminate
impressions of sound, and his muscles to the peculiar agility needed
for their regulated and delicate production; while, up to the age of
thirty-five, he had used his eyes no more purposefully than other
people. The eye, nevertheless, requires cultivation as much as the ear.
“You must not expect to _see at sight_,” he told Alexander Aubert, of
Loam Pit Hill, in 1782. And he wrote to Sir William Watson: “Seeing is
in some respects an art which must be learnt. Many a night have I been
practising to see, and it would be strange if one did not acquire a
certain dexterity by such constant practice.” A critical observation,
he added, could no more be expected from a novice at the telescope than
a performance of one of Handel’s organ-fugues from a beginner in music.
In this difficult art of vision he rapidly became an adept. Taking into
account the full extent of his powers, the opinion has been expressed,
and can scarcely be contradicted, that he never had an equal.

At midsummer, 1774, Herschel removed from No. 7, New King Street, to a
house situated near Walcot Turnpike, Bath. A grass-plot was attached
to the new residence, and it afforded convenient space for workshops.
For already he designed to “carry improvements in telescopes to their
utmost extent,” and “to leave no spot of the heavens unvisited.” An
unprecedented ambition! No son of Adam had ever before entertained
the like. To search into the recesses of space, to sound its depths,
to dredge up from them their shining contents, to classify these, to
investigate their nature, and trace their mutual relations, was what he
proposed to do, having first provided the requisite optical means. All
this in the intervals of professional toils, with no resources except
those supplied by his genius and ardour, with no experience beyond that
painfully gained during the progress of his gigantic task.

Since the time of Huygens, no systematic attempt had been made to add
to the power of the telescope. For the study of the planetary surfaces,
upon which he and his contemporaries were mainly intent, such addition
was highly desirable. But Newton’s discovery profoundly modified the
aims of astronomers. Their essential business then became that of
perfecting the theories of the heavenly bodies. Whether or not they
moved in perfect accordance with the law of gravitation was the crucial
question of the time. Newton’s generalisation was on its trial. Now and
again it almost seemed as if about to fail. But difficulties arose only
to be overcome, and before the eighteenth century closed the superb
mechanism of the planetary system was elucidated. Working flexibly
under the control of a single dominant force, it was shown to possess a
self-righting power which secured its indefinite duration. Imperishable
as the temple of Poseidon, it might be swayed by disturbances, but
could not be overthrown.

The two fundamental conclusions--that the Newtonian law is universally
valid, and that the solar system is a stable structure--were reached
by immense and sustained labours. Their establishment was due, in the
main, to the mathematical genius of Clairaut, D’Alembert, Lagrange,
and Laplace. But refined analysis demands refined data; hence the need
for increased accuracy of observation grew continually more urgent.
Attention was accordingly concentrated upon measuring, with the utmost
exactitude, the places at determinate epochs of the heavenly bodies.
The one thing needful was to learn the “when” and “where” of each of
them--that is, to obtain such information as the transit-instrument is
adapted to give. In this way the deviations of the moon and planets
from their calculated courses became known; and upon the basis of
these “errors” improved theories were built, then again compared with
corrected observations.

For these ends, large telescopes would have been useless. They were
not, however, those that Herschel had in view. The _nature_ of the orbs
around us, not their motions, formed the subject of his inquiries,
with which modern descriptive astronomy virtually originated. He was,
moreover, the founder of sidereal astronomy. The stars had, until
his career began, received little _primary_ attention. They were
regarded and observed simply as reference-points by which to track the
movements of planets, comets, and the moon. Indispensable for fiducial
purposes, they almost escaped consideration for themselves. They were,
indeed, thought to lie beyond the reach of effective investigation.
Only the outbursts of temporary stars, and the fluctuations of two
or three periodical ones, had roused special interest, and seemed
deserving of particular inquiry.

Of the dim objects called “nebulæ,” Halley had counted up half a
dozen in 1714; Lacaille compiled a list of forty-two at the Cape,
in 1752–55; and Messier published at Paris, in 1771, a catalogue of
forty-five, enlarged to one hundred and three in 1781. He tabulated,
only to rid himself of embarrassments from them. For he was _by trade_
a comet-hunter, and, until he hit upon this expedient, had been much
harassed in its exercise by mistakes of identity.

But Herschel did not merely “pick up;” he explored. This was what no
one before him had thought of doing. A “review of the heavens” was a
complete novelty. The magnificence of the idea, which was rooted in his
mind from the start, places him apart from, and above, all preceding
observers.

To its effective execution telescopic development was essential.
The two projects of optical improvement and of sidereal scrutiny
went together. The skies could be fathomed, if at all, only by means
of light-collecting engines of unexampled power. Rays enfeebled by
distance should be rendered effective by concentration. Stratum after
stratum of bodies--

     “Clusters and beds of worlds, and bee-like swarms
      Of suns and starry streams,”

previously unseen, and even unsuspected, might, by the strong focussing
of their feebly-surviving rays, be brought to human cognisance. The
contemplated “reviews” would then be complete just in proportion to the
grasp of the instrument used in making them.

The first was scarcely more than a reconnaissance. It was made in
1775, with a small reflector of the Newtonian make.[A] Its upshot was
to impress him with the utter disproportion between his daring plans
and the means as yet at his disposal. Speculum-casting accordingly
recommenced with fresh vigour. Seven- and ten-foot mirrors were
succeeded by others of twelve, and even of twenty feet focal length.
The finishing of them was very laborious. It was at that time a manual
process, during the course of which the hands could not be removed from
the metal without injury to its figure. One stretch of such work lasted
sixteen hours, Miss Herschel meantime, “by way of keeping him alive,”
putting occasional morsels of food into the diligent polisher’s mouth.
His mode of procedure was to cast and finish many mirrors of each
sort; then to select the best by trial, and repolish the remainder. In
this manner he made, before 1781, “not less than 200 seven-foot, 150
ten-foot, and about 80 twenty-foot mirrors, not to mention those of the
Gregorian form.” Repolishing operations were, moreover, accompanied
by constant improvements, so that each successive speculum tended to
surpass its predecessors.

    [A] In “Newtonian” telescopes the image formed by the large
        speculum is obliquely reflected from a small plane mirror
        to the side of the tube, where it is viewed with an
        ordinary eye-piece. With a “Gregorian,” the observer looks
        straight forward, the image being thrown back by a little
        _concave_ mirror through a central perforation in the
        speculum where the eye-piece is fitted.

These absorbing occupations were interrupted by the unwelcome news
that Dietrich, the youngest of the Herschel family, had decamped from
Hanover “with a young idler” like himself. William instantly started
for Holland, where the fugitive was supposed to be about to take
ship for India, but missed his track; and, after having extended his
journey to Hanover to comfort his anxious mother--his father had died
in 1767--returned sadly to Bath. There, to his immense surprise, he
found the scapegrace in strict charge of his sister, “who kept him to
a diet of roasted apples and barley-water.” His ineffectual escapade
had terminated with an attack of illness at Wapping, whither Alexander
Herschel, on learning how matters stood, had posted off to take him in
charge and watch his recovery. Musical occupation was easily procured
for him at Bath, since he was an accomplished violinist--had, indeed,
started on his unprosperous career in the guise of an infant prodigy;
but he threw it up in 1779 and drifted back to Hanover, married a Miss
Reif, and settled down to live out a fairly long term of shiftless,
albeit harmless, existence.

In 1776 William Herschel succeeded Thomas Linley, Sheridan’s
father-in-law, as Director of the Public Concerts at Bath. His duties
in this capacity, while the season lasted, were most onerous. He had to
engage performers, to appease discontents, to supply casual failures,
to write glees and catches expressly adapted to the voices of his
executants, frequently to come forward himself as a soloist on the
hautboy or the harpsichord. The services of his brother Alexander, a
renowned violoncellist, and of his sister, by this time an excellent
singer, were now invaluable to him. Nor for musical purposes solely.
The vision of the skies was never lost sight of, and the struggle
to realise it in conjunction with his sympathetic helpers absorbed
every remnant of time. At meals the only topics of conversation were
mechanical devices for improving success and averting failure. William
ate with a pencil in his hand, and a project in his head. Between the
acts at the theatre, he might be seen running from the harpsichord to
his telescope. After a rehearsal or a morning performance, he would
dash off to the workshop in periwig and lace ruffles, and leave it
but too often with those delicate adjuncts to his attire torn and
pitch-bespattered. Accidents, too, menacing life and limb, were a
consequence of that “uncommon precipitancy which accompanied all his
actions;” but he escaped intact, save for the loss of a finger-nail.

His introduction to the learned world of Bath was thus described by
himself:--

  “About the latter end of December, 1779, I happened to be
  engaged in a series of observations on the lunar mountains;
  and the moon being in front of my house, late in the evening I
  brought my seven-feet reflector into the street, and directed
  it to the object of my observations. Whilst I was looking into
  the telescope, a gentleman, coming by the place where I was
  stationed, stopped to look at the instrument. When I took my
  eye off the telescope, he very politely asked if he might be
  permitted to look in, and this being immediately conceded, he
  expressed great satisfaction at the view.”

The inquisitive stranger called next morning, and proved to be Dr.
(later Sir William) Watson. He formed on the spot an unalterable
friendship for the moon-struck musician, and introduced him to a
Philosophical Society which held its meetings at his father’s house.
Herschel’s earliest essays were read before it, but they remained
unpublished. His first printed composition appeared in the “Ladies’
Diary” for 1780. It was an answer to a prize question on the vibration
of strings.

The long series of his communications to the Royal Society of London
opened May 11th, 1780, with a discussion of his observations, begun in
October, 1777, of Mira, the variable star in the neck of the Whale. As
to the theory of its changes, he agreed with Keill that they could best
be explained by supposing rotation on an axis to bring a lucid side and
a side obscured by spots alternately into view. A second paper by him
on the Mountains of the Moon was read on the same day. He measured, in
all, about one hundred of these peaks and craters.

In January, 1781, there came an essay stamped with the peculiar impress
of his genius, entitled “Astronomical Observations on the Rotation of
the Planets round their Axes, made with a view to determine whether the
earth’s diurnal motion is perfectly equable.” It embodied an attempt to
apply a definite criterion to the time-keeping of our planet. But the
prospect is exceedingly remote of rating one planet-clock by the other.
Herschel’s methods of inquiry are, however, aptly illustrated in this
curiously original paper. His speculations always invited the control
of facts. If facts were not at hand, he tried somehow to collect them.
The untrammelled play of fancy was no more to his mind than it was to
Newton’s. His ardent scientific imagination was thus, by the sobriety
of his reason, effectively enlisted in the cause of progress.

Herschel began in 1780 his second review of the heavens, using a
seven-foot Newtonian, of 6¼ inches aperture, with a magnifying power
of 227. “For distinctness of vision,” he said, “this instrument is,
perhaps, equal to any that was ever made.” His praise was amply
justified. As he worked his way with it through the constellation
Gemini, on the night of March 13th, 1781, an unprecedented event
occurred. “A new planet swam into his ken.” He did not recognise it as
such. He could only be certain that it was not a fixed star. His keen
eye, armed with a perfect telescope, discerned at once that the object
had a disc; and the application of higher powers showed the disc to be
a substantial reality. The stellar “patines of bright gold” will not
stand this test. Being of purely optical production, they gain nothing
by magnification.

At that epoch new planets had not yet begun to be found by the dozen.
Five, besides the earth, had been known from the remotest antiquity.
Five, and no more, seemed to have a prescriptive right to exist. The
boundaries of the solar system were of immemorial establishment. It was
scarcely conceivable that they should need to be enlarged. The notion
did not occur to Herschel. His discovery was modestly imparted to the
Royal Society as “An Account of a Comet.” He had, indeed, noticed
that the supposed comet moved in planetary fashion from west to east,
and very near the ecliptic; and, after a few months, its true nature
was virtually proved by Lexell of St. Petersburg. On November 28th,
Herschel measured, with his freshly-invented “lamp-micrometer,” the
diameter of this “singular star;” and it was not until a year later,
November 7th, 1782, that he felt sufficiently sure of its planetary
status to exercise his right of giving it a name. Yet this, in the
long run, he failed to accomplish. The appellation “Georgium Sidus,”
bestowed in honour of his patron, George III., never crossed the
Channel, and has long since gone out of fashion amongst ourselves.
Lalande tried to get the new planet called “Herschel;” but the title
“Uranus,” proposed by Bode, of Berlin, was the “fittest,” and survived.

This discovery made the turning-point of Herschel’s career. It
transformed him from a music-master into an astronomer. Without it
his vast abilities would probably have been in great measure wasted.
No man could long have borne the strain of so arduous a double life
as he was then leading. Relief from it came just in time. It is true
that fame, being often more of a hindrance than a help, brought
embarrassments in its train. In November, 1781, Herschel was compelled
to break the complex web of his engagements at Bath by a journey to
London for the purpose of receiving in person the Copley Medal awarded
to him by the Royal Society, of which body he was, some days later,
elected a Fellow. At home, he was persecuted by admirers; and they
were invariably received with an easy suavity of manner that gave no
hint of preoccupation. Everyone of scientific pretension who visited
Bath sought an interview with the extraordinary man who, by way of
interlude to pressing duties, had built telescopes of unheard-of
power, and performed the startling feat of adding a primary member
to the solar system. Among the few of these callers whose names have
been preserved were Sir Harry Englefield, Sir Charles Blagden, and Dr.
Maskelyne, then, and for thirty years afterwards, Astronomer-Royal.
“With the latter,” Miss Herschel relates, “he (William) was engaged
in a long conversation which to me sounded like quarrelling, and the
first words my brother said after he was gone were, ‘That is a devil
of a fellow!’” The phrase was doubtless meant as a sign of regard, for
the acquaintance thus begun ripened into cordial intimacy. And William
Herschel never lost or forgot a friend.

As regards music alone, the winter of 1781–82 was an exceptionally busy
one. He had arranged to conduct, jointly with Rauzzini, a Roman singer
and composer, a series of oratorios; undertaking, besides, pecuniary
responsibilities which turned out little to his advantage. The labour,
vexation, and disappointment involved in carrying out this unlucky plan
can readily be imagined. But neither the pressure of business, nor
the distractions of celebrity, checked the ardour of his scientific
advance. The review which afforded him the discovery of Uranus, and the
materials for his first catalogue of 269 double stars, was completed
in 1781; and a third, made with the same beautiful instrument, bearing
the high magnifying power of 460, was promptly begun. This had for one
of its special objects the ascertainment of possible changes in the
heavens since Flamsteed’s time; and in the course of it many thousands
of stars came under scrutiny, directed to ascertain their magnitude and
colour, singleness or duplicity, hazy or defined aspect.

The first of Herschel’s _effective_ twenty-foot telescopes was erected
at 19, New King Street, in the summer of 1781. Enclosing a mirror
twelve inches in diameter, it far surpassed any seeing-machine that had
ever existed in the world. Yet its maker regarded it as only marking
a step in his upward progress. A speculum of thirty-feet focus was
the next object of his ambition. For its achievement no amount of
exertion was counted too great. Its composition was regulated by fresh
experiments on various alloys of copper and tin. Its weight and shape
were again and again calculated, and the methods appropriate to its
production earnestly discussed. “I saw nothing else,” Caroline Herschel
tells us, “and heard nothing else talked of but these things when my
brothers were together.”[B]

    [B] In borrowing Miss Herschel’s lively narratives and
        comments, some obvious slips in grammar and construction
        have been corrected. Quotations, too, from the writings
        of Sir William and Sir John Herschel are often slightly
        abridged.

“The mirror,” she continues, “was to be cast in a mould of loam
prepared from horse-dung, of which an immense quantity was to be
pounded in a mortar and sifted through a fine sieve. It was an endless
piece of work, and served me for many an hour’s exercise; and Alex
frequently took his turn at it, for we were all eager to do something
towards the great undertaking. Even Sir William Watson would sometimes
take the pestle from me when he found me in the work-room.”

The matter was never out of the master’s thoughts. “If a minute could
but be spared in going from one scholar to another, or giving one the
slip, he called at home to see how the men went on with the furnace,
which was built in a room below, even with the garden.”

At last, the concert season being over, and everything in readiness
for the operation of casting, “the metal,” we hear from the same
deeply-interested eyewitness, “was in the furnace; but, unfortunately,
it began to leak at the moment when ready for pouring, and both my
brothers, and the caster with his men, were obliged to run out at
opposite doors, for the stone flooring, which ought to have been taken
up, flew about in all directions, as high as the ceiling. My poor
brother William fell, exhausted with heat and exertion, on a heap of
brickbats. Before the second casting was attempted, everything which
could ensure success had been attended to, and a very perfect metal was
found in the mould, which had cracked in the cooling.”

This second failure terminated the enterprise. Not that it was
abandoned as hopeless, but because of a total change in the current of
affairs. Herschel’s fame had stirred the royal curiosity, and rumours
had now and again reached Bath that he was to be sent for to court. In
the spring of 1782 the actual mandate arrived; and on May 8th, leaving
his pupils and his projects to shift for themselves, he set out for
London. He carried with him his favourite seven-foot reflector, and all
the apparatus necessary for viewing double stars and other objects of
interest. On May 25th he wrote to his sister:--

“I have had an audience of His Majesty this morning, and met with a
very gracious reception. I presented him with the drawing of the solar
system, and had the honour of explaining it to him and the Queen. My
telescope is in three weeks’ time to go to Richmond, and meanwhile
to be put up at Greenwich.... Tell Alexander that everything looks
very like as if I were to stay here. The King enquired after him, and
after my great speculum. He also gave me leave to come and hear the
Griesbachs (Herschel’s nephews) play at the private concert which he
has every evening.... All my papers are printing, and are allowed to
be very valuable. You see, Lina, I tell you all these things. You
know vanity is not my foible, therefore I need not fear your censure.
Farewell.”

His next letter is dated June 3rd, 1782. “I pass my time,” he informed
“Lina,” “between Greenwich and London agreeably enough, but am rather
at a loss for work that I like. Company is not always pleasing, and I
would much rather be polishing a speculum. Last Friday I was at the
King’s concert to hear George play. The King spoke to me as soon as he
saw me, and kept me in conversation for half an hour. He asked George
to play a solo-concerto on purpose that I might hear him.... I am
introduced to the best company. To-morrow I dine at Lord Palmerston’s,
next day with Sir Joseph Banks, etc. Among opticians and astronomers
nothing now is talked of but _what they call_ my great discoveries.
Alas! this shows how far they are behind, when such trifles as I have
seen and done are called _great_. Let me but get at it again! I will
make such telescopes and see such things--that is, I will endeavour to
do so.”

A comparison of his telescope with those at the Royal Observatory
showed its striking superiority, although among them was one of Short’s
famous Gregorians, of 9½ inches aperture. It had thus a reflecting
surface above twice that of Herschel’s seven-foot, the competition
with which was nevertheless so disastrous to its reputation that Dr.
Maskelyne fell quite out of conceit with it, and doubted whether it
_deserved_ the new stand constructed for it on the model of Herschel’s.

In the midst of these scientific particulars, we hear incidentally that
influenza was then so rife in London that “hardly one single person”
escaped an attack.

On July 2nd he made his first appearance as showman of the heavens to
royalty. The scene of the display was Buckingham House (now Buckingham
Palace). “It was a very fine evening,” he wrote to his sister. “My
instrument gave general satisfaction. The King has very good eyes, and
enjoys observations with telescopes exceedingly.”

Next night, the King and Queen being absent at Kew, the Princesses
desired an exhibition. But, since they objected to damp grass, the
telescope, Herschel says, “was moved into the Queen’s apartments, and
we waited some time in hopes of seeing Jupiter or Saturn. Meanwhile
I showed the Princesses and several other ladies the speculum, the
micrometers, the movements of the telescope, and other things that
seemed to excite their curiosity. When the evening appeared to be
totally unpromising, I proposed an artificial Saturn as an object,
since we could not have the real one. I had beforehand prepared this
little piece, as I guessed by the appearance of the weather in the
afternoon we should have no stars to look at. This being accepted with
great pleasure, I had the lamps lighted up, which illuminated the
picture of a Saturn (cut out in pasteboard) at the bottom of the garden
wall. The effect was fine, and so natural that the best astronomer
might have been deceived. Their royal highnesses seemed to be much
pleased with the artifice.” From a somewhat prolonged conversation,
he judged them to be “extremely well instructed,” and “most amiable
characters.”

Shortly afterwards Herschel received the appointment of royal
astronomer, with the modest salary of £200 a year. “Never,” exclaimed
Sir William Watson on being made acquainted with its amount, “bought
monarch honour so cheap!” The provision was assuredly not munificent;
yet it sufficed to rescue a great man from submergence under the hard
necessities of existence. The offer was critically timed. It was made
precisely when teaching and concert-giving had come to appear an
“intolerable waste of time” to one fired with a visionary passion.
“Stout Cortes” staring at the Pacific, Ulysses starting from Ithaca to
“sail beyond the sunset,” were not more eager for experience of the
Unknown.




CHAPTER II.

THE KING’S ASTRONOMER.


William Herschel was now an appendage to the court of George III. He
had to live near Windsor, and a large dilapidated house on Datchet
Common was secured as likely to meet his unusual requirements. The
“flitting” took place August 1, 1782. William was in the highest
spirits. There were stables available for workrooms and furnaces; a
spacious laundry that could be turned into a library; a fine lawn for
the accommodation of the great reflector. Crumbling walls and holes
in the roof gave him little or no concern; and if butcher’s meat was
appallingly dear (as his sister lamented) the family could live on
bacon and eggs! In this sunny spirit he entered upon the career of
untold possibilities that lay before him.

Nevertheless the King’s astronomer did not find it all plain sailing.
His primary duty was to gratify the royal taste for astronomy, and this
involved no trifling expenditure of time and toil. The transport of the
seven-foot to the Queen’s lodge could be managed in the daylight, but
its return-journey in the dark, after the conclusion of the celestial
raree-show, was an expensive and a risky business; yet fetched back it
should be unless a clear night were to be wasted--a thing not possible
to contemplate. This kind of attendance was, however, considerately
dispensed with when its troublesome nature came to be fully understood.
Herschel’s treatment by George III. has often been condemned as
selfish and niggardly; but with scant justice. In some respects, no
doubt, it might advantageously have been modified. Still, the fact
remains that the astronomer of Slough was the gift to science of the
poor mad King. From no other crowned head has it ever received so
incomparable an endowment.

Herschel’s salary was undeniably small. It gave him the means of
living, but not of observing, as he proposed to observe. If the
improvement of telescopes were to be “carried to its utmost limit,”
additional funds must be raised. Without an ample supply of the “sinews
of war,” fresh campaigns of exploration were out of the question. There
was one obvious way in which they could be provided. Herschel’s fame as
an optician was spread throughout Europe. His telescopes were wanted
everywhere, but could be had from himself alone; for the methods by
which he wrought specula to a perfect figure are even now undivulged.
They constituted, therefore, a source of profit upon which he could
draw to almost any extent. He applied himself, accordingly, to make
telescopes for sale. They brought in large sums. Six hundred guineas
a-piece were paid to him by the King for four ten-foot reflectors; he
received at a later date £3,150 for a twenty-five foot, sent to Spain;
and in 1814 £2,310 from Lucien Bonaparte for two smaller instruments.
The regular scale of prices (later considerably reduced) began with 200
guineas for a seven-foot, and mounted to 2,500 for a twenty-foot; and
the commissions executed were innumerable.

But Herschel did not come into the world to drive a lucrative trade.
It was undertaken, not for itself, but for what was to come of it; yet
there was danger lest the end should be indefinitely postponed in the
endeavour to secure the means.

“It seemed to be supposed,” Miss Herschel remarked, “that enough had
been done when my brother was enabled to leave his profession that he
might have time to make and sell telescopes. But all this was only
retarding the work of a thirty or forty-foot instrument, which it was
his chief object to obtain as soon as possible; for he was then on the
wrong side of forty-five, and felt how great an injustice he would be
doing to himself and the cause of astronomy by giving up his time to
making telescopes for other observers.”

This he was, fortunately, not long obliged to do. A royal grant of
£2,000 for the construction of the designed giant telescope, followed
by another of equal amount, together with an annual allowance of
£200 for its repairs, removed the last obstacle to his success. The
wide distribution of first-class instruments might, indeed, have
been thought to promise more for the advancement of astronomy than
the labours of a single individual. No mistake could be greater. Not
an observation worth mentioning was made with any of the numerous
instruments sent out from Datchet or Slough, save only those acquired
by Schröter and Pond. The rest either rusted idly, or were employed
ineffectually, aptly illustrating the saying that “the man at the
eye-end” is the truly essential part of a telescope.

No one knew this better than Herschel. Every serene dark night was
to him a precious opportunity availed of to the last minute. The
thermometer might descend below zero, ink might freeze, mirrors might
crack; but, provided the stars shone, he and his sister worked on
from dusk to dawn. In this way, his “third review,” begun at Bath,
was finished in the spring of 1783. The swiftness with which it was
conducted implied no want of thoroughness. “Many a night,” he states,
“in the course of eleven or twelve hours of observation, I have
carefully and singly examined not less than 400 celestial objects,
besides taking measures, and sometimes viewing a particular star for
half an hour together, with all the various powers.”

The assiduity appears well-nigh incredible with which he gathered in
an abundant harvest of nebulæ and double stars; his elaborate papers,
brimful of invention and experience, being written by day, or during
nights unpropitious for star-gazing. On one occasion he is said to
have worked without intermission at the telescope and the desk for
seventy-two hours, and then slept unbrokenly for twenty-six hours. His
instruments were never allowed to remain disabled. They were kept,
like himself, on the alert. Relays of specula were provided, and one
was in no case removed from the tube for re-polishing, unless another
was ready to take its place. Even the meetings of the Royal Society
were attended only when moonlight effaced the delicate objects of his
particular search.

The summer of 1788 was spent in getting ready the finest telescope
Herschel had yet employed. It was called the “large twenty-foot”
because of the size of its speculum, which was nearly nineteen inches
in diameter; and with its potent help he executed his fourth and
last celestial survey. His impatience to begin led him into perilous
situations.

“My brother,” says Miss Herschel, “began his series of sweeps when the
instrument was yet in a very unfinished state; and my feelings were
not very comfortable when every moment I was alarmed by a crack or
fall, knowing him to be elevated fifteen feet or more on a temporary
cross-beam instead of a safe gallery. The ladders had not even their
braces at the bottom; and one night, in a very high wind, he had hardly
touched the ground before the whole apparatus came down. Some labouring
men were called up to help in extricating the mirror, which was
fortunately uninjured, but much work was cut out for carpenters next
day.”

In the following March, he himself wrote to Patrick Wilson, of Glasgow,
son of Dr. Alexander Wilson, the well-known professor of astronomy:--“I
have finished a second speculum to my new twenty-foot, very much
superior to the first, and am now reviewing the heavens with it. This
will be a work of some years; but it is to me so far from laborious
that it is attended with the utmost delight.” He, nevertheless, looked
upon telescopes as “yet in their infant state.”

The ruinous mansion at Datchet having become uninhabitable, even
by astronomers, their establishment was shifted, in June, 1785, to
Clay Hall, near Old Windsor. Here the long-thought-of forty-foot was
begun, but was not destined to be finished. A litigious landlady
intervened. The next move, however, proved to be the last. It was to
a commodious residence at Slough, now called “Observatory House”--“le
lieu du monde,” wrote Arago, “où il a été fait le plus de découvertes.”
Thither, without the loss of an hour, in April, 1786, the machinery and
apparatus collected at Clay Hall were transported. Yet, “amidst all
this hurrying business,” Caroline remembered “that every moment after
daylight was allotted to observing. The last night at Clay Hall was
spent in sweeping till daylight, and by the next evening the telescope
stood ready for observation at Slough.”

During the ensuing three months, thirty to forty workmen were
constantly employed, “some in felling and rooting out trees, some in
digging and preparing the ground for the bricklayers who were laying
the foundation for the telescope.” “A whole troop of labourers” were,
besides, engaged in reducing “the iron tools to a proper shape for the
mirror to be ground upon.” Thus, each morning, when dawn compelled
Herschel to desist from observation, he found a bevy of people awaiting
instructions of all sorts from him. “If it had not been,” his sister
says, “for the intervention of a cloudy or moonlit night, I know not
when he, or I either, should have got any sleep.” The wash-house was
turned into a forge for the manufacture of specially designed tools;
heavy articles cast in London were brought by water to Windsor; the
library was so encumbered with stores, models, and implements, that “no
room for a desk or an atlas remained.”

On July 3rd, 1786, Herschel, accompanied by his brother Alexander,
started for Göttingen, commissioned by the King to present to the
University one of the ten-foot reflectors purchased from him. He was
elected a Member of the Royal Society of Göttingen, and spent three
weeks at Hanover with his aged mother, whom he never saw again. During
his absence, however, the forty-foot progressed in accordance with
the directions he had taken care to leave behind. He trusted nothing
to chance. “There is not one screwbolt,” his sister asserted, “about
the whole apparatus but what was fixed under the immediate eye of
my brother. I have seen him lie stretched many an hour in a burning
sun, across the top beam, whilst the iron-work for the various motions
was being fixed. At one time no less than twenty-four men (twelve and
twelve relieving each other) kept polishing day and night; my brother,
of course, never leaving them all the while, taking his food without
allowing himself time to sit down to table.”

At this stage of the undertaking it became the fashion with visitors to
use the empty tube as a promenade. Dr. and Miss Burney called, in July,
1786, “to see, and _take a walk_ through the immense new telescope.”
“It held me quite upright,” the authoress of “Evelina” related, “and
without the least inconvenience; so would it have done had I been
dressed in feathers and a bell-hoop.”

George III. and the Archbishop of Canterbury followed the general
example; and the prelate being incommoded by the darkness and the
uncertain footing, the King, who was in front, turned back to help him,
saying: “Come, my lord bishop, I will show you the way to heaven.” On
another occasion “God save the King” was sung and played within the
tube by a large body of musicians; and the rumour went abroad that it
had been turned into a ball-room!

The University of Oxford conferred upon Herschel, in 1786, an honorary
degree of LL.D.; but he cared little for such distinctions. Miss
Burney characterised him as a “man without a wish that has its object
in the terrestrial globe;” the King had “not a happier subject.” The
royal bounty, she went on “enables him to put into execution all his
wonderful projects, from which his expectations of future discoveries
are so sanguine as to make his present existence a state of almost
perfect enjoyment.” Nor was it possible to “admire his genius more
than his gentleness.” Again, after taking tea in his company in the
Queen’s lodge: “this very extraordinary man has not more fame to
awaken curiosity than sense and modesty to gratify it. He is perfectly
unassuming, yet openly happy; and happy in the success of those studies
which would render a mind less excellently formed presumptuous and
arrogant.” Mrs. Papendick, another court chronicler, says that “he was
fascinating in his manner, and possessed a natural politeness, and the
abilities of a superior nature.”

His great telescope took rank, before and after its completion, as the
chief scientific wonder of the age. Slough was crowded with sightseers.
All the ruck of Grand Dukes and Serene Highnesses from abroad, besides
royal, noble, and gentle folk at home, flocked to gaze at it and
interrogate its maker with ignorant or intelligent wonder. The Prince
of Orange was a particularly lively inquirer. On one of his calls at
Slough, about ten years after the erection of the forty-foot, finding
the house vacant, he left a memorandum asking if it were true, as the
newspapers reported, that “Mr. Herschel had discovered a new star whose
light was not as that of the common stars, but with swallow-tails, as
stars in embroidery?”!

Pilgrim-astronomers came, too--Cassini, Lalande, Méchain and Legendre
from Paris, Oriani from Milan, Piazzi from Palermo. Sniadecki, director
of the observatory of Cracow, “took lodgings,” Miss Herschel relates,
“in Slough, for the purpose of seeing and hearing my brother whenever
he could find him at leisure. He was a very silent man.” One cannot
help fearing that he was also a very great bore. Von Magellan, another
eminent foreign astronomer, communicated to Bode an interesting account
of Herschel’s methods of observation. The multitude of entries in his
books astonished him. In sweeping, he reported, “he lets each star pass
at least three times through the field of his telescope, so that it is
impossible that anything can escape him.” The thermometer in the garden
stood that night, January 6th, 1785, at 13 deg. Fahrenheit; but the
royal astronomer, his visitor remarked, “has an excellent constitution,
and thinks about nothing else in the world but the celestial bodies.”

In January, 1787, Herschel made trial with his twenty-foot reflector
of the “front-view” plan of construction, suggested by Lemaire in
1732, but never before practically tested. All that had to be done
was to remove the small mirror, and slightly _tilt_ the large one.
The image was then formed close to the upper margin of the tube, into
which the observer, turning his back to the heavens, looked down. The
purpose of the arrangement was to save the light lost in the second
reflection; and its advantage was at once illustrated by the discovery
of two Uranian moons--one (Titania) circling round its primary in about
8¾ hours, the other (Oberon) in 13½ hours. In order to assure these
conclusions, he made a sketch beforehand of what _ought_ to be seen on
February 10th; and on that night, to his intense satisfaction, “the
heavens,” as he informed the Royal Society, “displayed the original of
my drawing by showing, in the situation I had delineated them, _the
Georgian planet attended by two satellites_. I confess that this scene
appeared to me with additional beauty, the little secondary planets
seeming to give a dignity to the primary one which raises it into a
more conspicuous situation among the great bodies of our solar system.”

This brilliant result determined him to make a “front-view” of
the forty-foot. Its advance towards completion was not without
vicissitudes. The first speculum, when put into the tube, February
19th 1787, was found too thin to maintain its shape. A second, cast
early in 1788, cracked in cooling. The same metal having been recast
February 16th, the artist tried it upon Saturn in October; but the
effect disappointing his expectation, he wrought at it for ten months
longer. At last, after a few days’ polishing with his new machine, he
turned the great speculum towards Windsor Castle; when its high quality
became at once manifest. And such was his impatience to make with it
a crucial experiment, that--as he told Sir Joseph Banks--he directed
it to the heavens (August 28th, 1789) before it had half come to its
proper lustre. The stars came out well, and no sooner had he got hold
of Saturn than a sixth satellite stood revealed to view! Its “younger
brother” was detected September 17th; and the two could be seen, on
favourable opportunities, threading their way, like beads of light,
along the lucid line of the almost vanished ring. Herschel named them
Enceladus and Mimas, and found, on looking up his former observations
of Saturn, that Enceladus, the exterior and brighter object, had been
unmistakably seen with the twenty-foot, August 19th, 1787. Mimas is a
very delicate test of instrumental perfection.

The mirror by which it was first shown measured nearly fifty inches
across, and weighed 2,118 pounds. It was slung in a ring, and the
sheet-iron tube in which it rested was thirty-nine and a-half feet
long and four feet ten inches wide. Ladders fifty feet in length
gave access to a movable stage, from which the observer communicated
through speaking tubes with his assistants. The whole erection stood
on a revolving platform; for the modern equatorial form of mount, by
which the diurnal course of the heavens is automatically followed, was
not then practically available, and the necessary movements had to be
imparted by hand. This involved the attendance of two workmen, but was
otherwise less inconvenient than might be supposed, owing to the skill
with which the required mechanism was contrived.

Herschel estimated that, with a magnifying-power of 1,000, this grand
instrument could, in the climate of England, be effectively used during
no more than one hundred hours of every year. A review with it of the
whole heavens would hence have occupied eight centuries. In point of
fact, he found the opportunities for its employment scarce. The machine
took some time to get started, while the twenty-foot was ready in ten
minutes. The speculum, moreover, proved unpleasantly liable to become
dewed in moist weather, or frozen up in cold; and, in spite of all
imaginable care, it preserved the delicacy of its polish no more than
two years. An economist of minutes, such as its maker, could, then,
do no otherwise than let the giant telescope lie by unless its powers
were expressly needed. They were surprisingly effective. “With the
forty-foot instrument,” he reported to the Royal Society in 1800, “the
appearance of Sirius announced itself at a great distance like the dawn
of the morning, till this brilliant star at last entered the field,
with all the splendour of the rising sun, and forced me to take my eye
from that beautiful sight.” Which, however, left the vision impaired
in delicacy for nigh upon half-an-hour.

Thus the results gathered from the realisation of Herschel’s crowning
optical achievement fell vastly short of what his imagination had
pictured. The promise of the telescope’s initial disclosures was not
realised in its subsequent career. Yet it was a superb instrument.
The discovery with it of Mimas gave certain proof that the figure of
the speculum was as perfect as its dimensions were unusual. But its
then inimitable definition probably fell off later. Its “broad bright
eye” was, for the last time, turned towards the heavens January 19th,
1811, when the Orion nebula showed its silvery wings to considerable
advantage. But incurable dimness had already set in--incurable, because
the artist’s hand had no longer the strength needed to cure the growing
malady. The big machine was, however, left standing, framework and all.
It figured as a landmark on the Ordnance Survey Map of England; and,
stamped in miniature on the seal of the Royal Astronomical Society,
aptly serves to illustrate its motto, “_Quicquid nitet notandum_.”
At last, on New Years Eve, 1839, the timbers of the scaffolding
being dangerously decayed, it was, with due ceremony, dismounted. A
“Requiem,” composed by Sir John Herschel, was sung by his family,
fourteen in number, assembled within the tube, which was then riveted
up and laid horizontally on three stone piers in the garden at Slough.
“It looks very well in its new position,” Sir John thought. Yet it has
something of a _memento mori_ aspect. It seems to remind one that the
loftiest human aspirations are sprinkled “with the dust of death.” The
speculum adorns the hall of Observatory House.

Herschel married, May 8th, 1788, Mary, the only child of Mr. James
Baldwin, a merchant in the City of London, and widow of Mr. John Pitt.
She was thirty-eight and he fifty. Her jointure relieved him from
pecuniary care, and her sweetness of disposition secured his domestic
happiness. They set up a curious double establishment, taking a house
at Upton, while retaining that at Slough. Two maidservants were kept
in each, and a footman maintained the communications. So at least runs
Mrs. Papendick’s gossip. Miss Burney records in her Diary a tea at Mr.
De Luc’s, where Dr. Herschel accompanied a pair of vocalists “very
sweetly on the violin. His newly-married wife was with him, and his
sister. His wife seems good-natured; she was rich, too! And astronomers
are as able as other men to discern that gold can glitter as well as
stars.”

He was now at the height of prosperity and renown. Diplomas innumerable
were showered upon him by Academies and learned societies. In a letter
to Benjamin Franklin, he returned thanks for his election as a member
of the American Philosophical Society, and acquainted him with his
recent detection of a pair of attendants on the “Georgian planet.”
A similar acknowledgment was addressed to the Princess Daschkoff,
Directress of the Petersburg Academy of Sciences. The King of Poland
sent him his portrait; the Empress Catherine II. opened negotiations
for the purchase of some of his specula, Lucien Bonaparte repaired
to Slough incognito; Joseph Haydn snatched a day from the turmoil
of his London engagements to visit the musician-astronomer, and
gaze at his monster telescopes. By universal agreement, Dr. Burney
declared, Herschel was “one of the most pleasing and well-bred natural
characters of the day, as well as the greatest astronomer.” They had
much in common, according to Dr. Burney’s daughter. Both possessed an
uncommon “suavity of disposition”; both loved music; and Dr. Burney had
a “passionate inclination for astronomy.” They became friends through
the medium of Dr. Burney’s versified history of that science. In
September, 1797, he called at Slough with the manuscript in his valise.
“The good soul was at dinner,” he relates; and, to his surprise, since
he was ignorant of Herschel’s marriage, the company included several
ladies, besides “a little boy.” He was, nothing loth, compelled to stay
over-night; discussed with his host the plan of his work, and read to
him its eighth chapter. Herschel listened with interest, and modestly
owned to having learnt much from what he had heard; but presently
dismayed the author by confessing his “aversion to poetry,” which
he had generally regarded as “an arrangement of fine words without
any adherence to the truth.” He added, however, that “when truth and
science were united to those fine words,” they no longer displeased
him. The readings continued at intervals, alternately at Slough and
Chelsea, to the immense gratification of the copious versifier, who
occasionally allowed his pleasure to overflow in his correspondence.

“Well, but Herschel has been in town,” he wrote from Chelsea College,
December 10th, 1798, “for short spurts and back again, two or three
times, and I have had him here two whole days. I read to him the first
five books without any one objection.” And again; “He came, and his
good wife accompanied him, and I read four and a-half books; and on
parting, still more humble than before, or still more amiable, he
thanked me for the instruction and entertainment I had given him. What
say you to that? Can anything be grander?”

In spite of his “aversion,” Herschel had once, and once only, wooed the
coy muse himself. The first evening paper that appeared in England, May
3rd, 1788, contained some introductory quatrains by him. An excuse for
this unwonted outburst may be found in the circumstance that the sheet
in which they were printed bore the name of _The Star_. They began with
the interrogation:

     “What Star art thou, about to gleam
        In Novelty’s bright hemisphere?”

and continued:

     “A Planet wilt thou roll sublime,
        Spreading like Mercury thy rays?
      Or chronicle the lapse of Time,
        Wrapped in a Comet’s threatening blaze?”

That they are of the schoolboy order need surprise no one. Such a mere
sip at the “Pierian spring” could scarcely bring inspiration.

Herschel’s grand survey of the heavens closed with his fourth review.
His telescopic studies thereupon became specialised. The sun, the
planets and their satellites, the lately discovered asteroids, certain
double stars, and an occasional comet, in turn received attention.
Laboratory experiments were also carried on, and discussions of
profound importance were laid before the Royal Society. All this
cost him but little effort. The high tension of his earlier life was
somewhat relaxed; he allowed himself intervals of rest, and indulged
in social and musical recreations. Concerts were now frequently given
at his house; and the face of beaming delight with which he presided
over them is still traditionally remembered. Visits to Sir William
Watson at Dawlish gave him opportunities, otherwise rare, for talks on
metaphysical subjects; and he stayed with James Watt at Heathfield in
1810. He had been a witness on his side in an action for infringement
of patent in 1793.

Herschel rented a house on Sion Hill, Bath, for some months of the year
1799; and from time to time stayed with friends in London, or sought
change of air at Tunbridge Wells, Brighton, or Ramsgate. In July,
1801, he went to Paris with his wife and son, made acquaintance with
Laplace, and had an interview with the First Consul. It was currently
reported that Bonaparte had astonished him by the extent of his
astronomical learning; but the contrary was the truth. He had tried to
be impressive, but failed. Herschel gave an account of what passed to
the poet Campbell, whom he met at Brighton in 1813.

“The First Consul,” he said, “did surprise me by his quickness and
versatility on all subjects; but in science he seemed to know little
more than any well-educated gentleman; and of astronomy much less,
for instance, than our own king. His general air was something like
affecting to know more than he did know.” Herschel’s election in 1802
as one of the eight foreign Associates of the French Institute was
probably connected with his Parisian experiences.

He inspired Campbell with the most lively enthusiasm. “His simplicity,”
he wrote, “his kindness, his anecdotes, his readiness to explain--and
make perfectly conspicuous too--his own sublime conceptions of the
universe, are indescribably charming. He is seventy-six, but fresh
and stout; and there he sat, nearest the door at his friend’s house,
alternately smiling at a joke, or contentedly sitting without share
or notice in the conversation. Any train of conversation he follows
implicitly; anything you ask, he labours with a sort of boyish
earnestness to explain. Speaking of himself, he said, with a modesty of
manner which quite overcame me, when taken together with the greatness
of the assertion, ‘I have looked further into space than ever human
being did before me; I have observed stars, of which the light, it can
be proved, must take two millions of years to reach this earth.’ I
really and unfeignedly felt at the moment as if I had been conversing
with a supernatural intelligence. ‘Nay, more,’ said he, ‘if those
distant bodies had ceased to exist two millions of years ago we should
still see them, as the light would travel after the body was gone.’
These were Herschel’s words; and if you had heard him speak them, you
would not think he was apt to tell more than the truth.”

The appearance of a bright comet, in October, 1806, drew much company
to Slough. On the 4th, Miss Herschel narrates, “Two parties from the
Castle came to see it, and during the whole month my brother had not
an evening to himself. As he was then in the midst of polishing the
forty-foot mirror, rest became absolutely necessary after a day spent
in that most laborious work; and it has ever been my opinion that on
the 14th of October his nerves received a shock from which he never
got the better afterwards; for on that day he had hardly dismissed
his troop of men when visitors assembled, and from the time it was
dark, till past midnight, he was on the grass-plot surrounded by
between fifty and sixty persons, without having had time to put on
proper clothing, or for the least nourishment to pass his lips. Among
the company I remember were the Duke of Sussex, Prince Galitzin, Lord
Darnley, a number of officers, Admiral Boston, and some ladies.”

A dangerous attack of illness in the spring of 1807 left Herschel’s
strength permanently impaired. But he travelled to Scotland in the
summer of 1810, and received the freedom of the City of Glasgow.
Then, in 1814, he made a final, but fruitless attempt, to renovate
the four-foot speculum. In the midst of the confusion attending upon
the process, word was given to prepare for the reception of the Czar
Alexander, the Duchess of Oldenburg, and sundry other grandees just
then collected at Windsor for the Ascot races. The setting to rights
was no small job; “but we might have saved ourselves the trouble,” his
sister remarks drily, “for they were sufficiently harassed with public
sights and festivities.”

On April 5th, 1816, Herschel was created a Knight of the Royal
Hanoverian Guelphic Order, and duly attended one of the Prince Regent’s
levées in May. He went to town in 1819 to have his portrait painted
by Artaud. The resulting fine likeness is in the possession of his
grandson, Sir William James Herschel. The Astronomical Society chose
him as its first President in 1821; and he contributed to the first
volume of its memoirs a supplementary list of 145 double stars. The
wonderful series of his communications to the Royal Society closed
when he was in his eightieth year, with the presentation, June 11th,
1818, of a paper on the Relative Distances of Star-clusters. On June
1st, 1821, he inserted into the tube with thin and trembling hands
the mirror of the twenty-foot telescope, and took his final look at
the heavens. All his old instincts were still alive, only the bodily
power to carry out their behests was gone. An unparalleled career of
achievement left him unsatisfied with what he had done. Old age brought
him no Sabbath rest, but only an enforced and wearisome cessation from
activity. His inability to re-polish the four-foot speculum was the
doom of his _chef d’œuvre_. He could not reconcile himself to it. His
sunny spirits gave way. The old happy and buoyant temperament became
overcast with despondency. His strong nerves were at last shattered.

On August 15th, 1822, Miss Herschel relates:--“I hastened to the spot
where I was wont to find him with the newspaper I was to read to him.
But I was informed my brother had been obliged to return to his room,
whither I flew immediately. Lady Herschel and the housekeeper were with
him, administering everything which could be thought of for supporting
him. I found him much irritated at not being able to grant Mr.
Bulman’s[C] request for some token of remembrance for his father. As
soon as he saw me, I was sent to the library to fetch one of his last
papers and a plate of the forty-foot telescope. But for the universe I
could not have looked twice at what I had snatched from the shelf, and
when he faintly asked if the breaking-up of the Milky Way was in it,
I said ‘Yes,’ and he looked content. I cannot help remembering this
circumstance; it was the last time I was sent to the library on such
an occasion. That the anxious care for his papers and workrooms never
ended but with his life, was proved by his whispered inquiries if they
were locked, and the key safe.”

    [C] The grandson of one of Herschel’s earliest English friends.

He died ten days later, August 25th, 1822. Above his grave, in the
church of Saint Laurence at Upton, the words are graven:--“Coelorum
perrupit claustra”--He broke through the barriers of the skies.

William Herschel was endowed by nature with an almost faultless
character. He had the fervour, without the irritability of genius; he
was generous, genial, sincere; tolerant of ignorance; patient under the
acute distress, to which his situation rendered him peculiarly liable,
of unseasonable interruptions at critical moments: he was warm-hearted
and open-handed. His change of country and condition, his absorption
in science, the homage paid to him, never led him to forget the claims
of kindred. Time and money were alike lavished in the relief of family
necessities. He supported his brother Alexander after his retirement
from the concert-stage in 1816, until his death at Hanover, March 15th,
1821. Dietrich’s recurring misfortunes met his unfailing pity and
help. He bequeathed to him a sum of £2,000, and to his devoted sister,
Caroline, an annuity of £100.

His correspondents, abroad and at home, were numerous; nor did he
disdain to remove the perplexities of amateurs. In a letter, dated
January 6th, 1794, we find him explaining to Mr. J. Miller of Lincoln’s
Inn, “the circumstances which attend the motion of a race-horse upon
a circle of longitude.” And he wrote shortly afterwards to Mr. Smith
of Tewkesbury:--“You find fault with the principles of gravitation
and projection because they will not account for the rotation of the
planets upon their axes. You might certainly with as much reason find
fault with your shoes because they will not likewise serve your hands
as gloves. But, in my opinion, the projectile motion once admitted,
sufficiently explains the rotatory motion; for it is hardly possible
mechanically to impress the one without giving the other at the same
time.”

On religious topics he was usually reticent; but a hint of the reverent
spirit in which his researches were conducted may be gathered from
a sentence in the same letter. “It is certainly,” he said, “a very
laudable thing to receive instruction from the great workmaster of
nature, and for that reason all experimental philosophy is instituted.”

To investigate was then, in his view, to “receive instruction”; and one
of the secrets of his wonderful success lay in the docility with which
he came to be taught.




CHAPTER III.

THE EXPLORER OF THE HEAVENS.


“A knowledge of the construction of the heavens,” Herschel wrote
in 1811, “has always been the ultimate object of my observations.”
The “Construction of the Heavens”! A phrase of profound and novel
import, for the invention of which he was ridiculed by Brougham in the
_Edinburgh Review_; yet expressing, as it had never been expressed
before, the essential idea of sidereal astronomy. Speculation there had
been as to the manner in which the stars were grouped together; but the
touchstone of reality had yet to be applied to them. This unattempted,
and all but impossible enterprise Herschel deliberately undertook. It
presented itself spontaneously to his mind as worth the expenditure
of a life’s labour; and he spared nothing in the disbursement. The
hope of its accomplishment inspired his early exertions, carried him
through innumerable difficulties, lent him audacity, fortified him in
perseverance. For this,

     “He left behind the painted buoy
        That tosses at the harbour’s mouth,”

and burst his way into an unnavigated ocean.

Herschel has had very few equals in his strength of controlled
imagination. He held the balance, even to a nicety, between the
real and the ideal. Meditation served in him to prescribe and guide
experience; experience to ripen the fruit of meditation.

“We ought,” he wrote in 1785, “to avoid two opposite extremes. If we
indulge a fanciful imagination, and build worlds of our own, we must
not wonder at our going wide from the path of truth and nature. On the
other hand, if we add observation to observation without attempting to
draw, not only certain conclusions, but also conjectural views from
them, we offend against the very end for which only observations ought
to be made.”

This was consistently his method. If thought outran sight, he laboured
earnestly that it should be overtaken by it: while sight, in turn,
often took the initiative, and suggested thought. He was much more than
a simple explorer. “Even at the telescope,” Professor Holden says, “his
object was not discovery merely, but to know the inner constitution of
the heavens.” He divined, at the same time that he observed.

The antique conception of the heavens as a hollow sphere upon which
the celestial bodies are seen projected, survived then, and survives
now, as a convenient fiction for practical purposes. But in the
eighteenth century the fiction assumed to the great majority a sort of
quasi-reality. Herschel made an exception in being vividly impressed
with the _depth_ of space. How to sound that depth was the first
problem that he attacked. As a preliminary to further operations, he
sought to fix a unit of sidereal measurement. The distances from the
earth to the stars were then altogether unknown. All that had been
ascertained was that they must be very great. Instrumental refinements
had not, in fact, been carried far enough to make the inquiry
profitable. Herschel did not underrate its difficulty. He recognised
that, in pursuing it, _one hundredth of a second of arc_ “became a
quantity to be considered.” Justly arguing, however, that previous
experiments on stellar parallax had been unsatisfactory and indecisive,
he determined to try again.

He chose the “double star method,” invented by Galileo, but never, so
far, effectually put to trial. The principle of it is perfectly simple,
depending upon the perspective shifting to a spectator in motion, of
objects at different distances from him. In order to apprehend it,
one need only walk up and down before a lamp placed in the middle of
a room, watching its apparent change of position relative to another
lamp at the end of the same room. Just in the same way, a star observed
from opposite sides of the earth’s orbit is sometimes found to alter
its situation very slightly by comparison with another star close to it
in the sky, but indefinitely remote from it in space. Half the small
oscillation thus executed is called that star’s “annual parallax.” It
represents the minute angle under which the radius of the terrestrial
orbit would appear at the star’s actual distance. So vast, however, is
the scale of the universe, that this tell-tale swing to and fro is,
for the most part, imperceptible even with modern appliances, and was
entirely inaccessible to Herschel’s observations. Yet they did not
remain barren of results.

“As soon as I was fully convinced,” he wrote in 1781, “that in the
investigation of parallax the method of double stars would have many
advantages above any other, it became necessary to look out for proper
stars. This introduced a new series of observations. I resolved to
examine every star in the heavens with the utmost attention that I
might fix my observations upon those that would best answer my end.
The subject promises so rich a harvest that I cannot help inviting
every lover of astronomy to join with me in observations that must
inevitably lead to new discoveries. I took some pains to find out
what double stars had been recorded by astronomers; but my situation
permitted me not to consult extensive libraries, nor, indeed, was it
very material; for as I intended to view the heavens myself, Nature,
that great volume, appeared to me to contain the best catalogue.”

On January 10th, 1782, he presented to the Royal Society a catalogue
of 269 double stars, of which 227 were of his own finding; and a
second list of 434 followed in December, 1784. All were arranged in
six classes, according to the distance apart of their components,
ranging from one up to 120 seconds. The close couples he regarded as
especially adapted for parallax-determinations; the wider ones might
serve for criteria of stellar proper movements, or even of the sun’s
transport through space. For the purpose of measuring the directions
in which their members lay towards each other--technically called
“position-angles”--and the intervals separating them, he invented
two kinds of micrometers, and notes were added as to their relative
brightness and colours. He was the first to observe the lovely
contrasted or harmonised tints displayed by some of these objects.

Herschel’s double stars actually fulfilled none of the functions
assigned to them. He was thus left without any definite unit of
measurement for sidereal space; and he never succeeded in supplying the
want. In 1814 he was “still engaged,” though vainly, “in ascertaining
a scale whereby the extent of the universe, so far as it is possible
for us to penetrate into space, may be fathomed.” He knew only that
the distances of the stars nearest the earth could not be less, and
might be a great deal more, than light-waves, propagated at the rate
of 186,300 miles a second, would traverse in three or four years. Only
the _manner_ of stellar arrangement, then, remained open to his zealous
investigations.

The initial question presenting itself to an intelligent spectator of
the nocturnal sky is: What relation does the dim galactic star-stream
bear to the constellations amidst which it flows? And this question
our interior position makes very difficult to be answered. We see
the starry universe, it has been well said, “not in _plan_ but in
_section_.” The problem is, from that section to determine the plan--to
view the whole mentally as it would show visually from the outside. The
general appearance to ourselves of the Milky Way leaves it uncertain
whether it represents the projection upon the heavens of an immense
stratum of equally scattered stars, or a ring-like accumulation,
towards the middle of which our sun is situated. Herschel gave his
preference, to begin with, to the former hypothesis, and then, with
astonishing boldness and ingenuity, attempted to put it experimentally
to the proof.

His method of “star-gauging” was described in 1784. It consisted in
counting the stars visible in successive fields of his twenty-foot
telescope, and computing the corresponding depths of space. Admitting
an average regularity of distribution, this was easily done. If the
stars did not really lie closer together in one region than in another,
then the more of them there were to be seen along a given line of
vision, the further the system could be inferred to extend in that
particular direction. The ratio of its extension would also be given.
It would vary with the cube-roots of the number of stars in each count.

Guided by this principle, Herschel ventured to lay down the boundaries
of the stellar aggregation to which our sun belongs. So far as he
“had yet gone round it,” in 1785, he perceived it to be “everywhere
terminated, and in most places very narrowly too.” The differences,
however, between his enumerations in various portions of the sky
were enormous. In the Milky Way zone the stars presented themselves
in shoals. He met fields--of just one quarter the area of the
moon--containing nearly 600; so that, in fifteen minutes, 116,000
were estimated to have marched past his stationary telescope. Here,
the calculated “length of his sounding-line” was nearly 500 times the
distance of Sirius, his standard star. Towards the galactic poles, on
the contrary, stars were comparatively scarce; and the transparent
blackness of the sky showed that in those quarters the supply of
stars was completely exhausted. At right angles to the Milky Way,
then, the stellar system might be termed shallow, while in its plane,
it stretched out on all sides to an inconceivable, though not to an
illimitable extent. Its shape appeared, accordingly, to be that of a
flat disc, of very irregular contour, and with a deep cleft matching
the bifid section of the Milky Way between Cygnus and Scorpio.

Herschel regarded this conclusion only “as an example to illustrate
the method.” Yet it was derived from the reckoning-up of 90,000 stars
in 2,400 telescopic fields! Its validity rested on the assumption
that stellar crowding indicated, not more stars in a given space, but
more space stocked in the same proportion with stars. But his hope
of thus getting a true mean result collapsed under the weight of his
own observations. “It would not be difficult,” he stated in 1785, “to
point out two or three hundred gathering clusters in our system.” The
action of a “clustering power” drawing its component stars “into many
separate allotments” grew continually clearer to him, and he admitted
unreservedly in 1802 that the Milky Way “consists of stars very
differently scattered from those immediately about us.”

In 1811, he expressly abandoned his original hypothesis. “I must freely
confess,” he wrote, “that by continuing my sweeps of the heavens
my opinion of the arrangement of the stars has undergone a gradual
change. An equal scattering of the stars may be admitted in certain
calculations; but when we examine the Milky Way, or closely compressed
clusters, it must be given up.”

And in 1817: “Gauges, which on a supposition of an equality of
scattering, were looked upon as gauges of distance, relate, in fact,
more immediately to the scattering of the stars, of which they give
valuable information.”

The “disc-theory” was then virtually withdrawn not many years after it
had been propounded. “The subtlety of nature,” according to Bacon’s
aphorism, “transcends the subtlety both of the intellect and of the
senses.” Herschel very soon perceived the inadequacy of his colossal
experiment; and he tranquilly acquiesced, not being among those who
seek to entrench theory against evidence. He found that he had
undervalued the complexity of the problem. Yet it remained before his
mind to the end. The supreme object of his scientific life was to
ascertain the laws of stellar distribution in cubical space, and he
devoted to the subject the two concluding memoirs of the sixty-nine
contributed by him to the “Philosophical Transactions.” He was in his
eightieth year when he opened, with youthful freshness, a new phase of
arduous investigation.

“The construction of the heavens,” he wrote in June, 1817, “can only
be known when we have the situation of each body defined by its three
dimensions. Of these three, the ordinary catalogues give but two,
leaving the distance or profundity undetermined.” This element of
“profundity” he went on to determine by the absolutely novel method of
what may be called “photometric enumeration.”

He began by asserting what is self-evident--that faint stars are, “one
with another,” more remote than bright ones; and he argued thence,
reasonably enough, that the relative mean distances of the stars, taken
order by order, might be inferred from their relative mean magnitudes.
Next he pointed out that more space would be available for their
accommodation in proportion to the cubes of their mean distances.
Here lies the value of the method. It sets up, as Herschel said, “a
standard of reference” with regard to stellar distribution. It makes it
possible to compare actual stellar density, at a given mean distance,
with a “certain properly modified equality of scattering.” By patiently
calling over the roll of successive magnitudes, information may be
obtained regarding over- and under-populated districts of space.

Herschel’s reasonings on the subject are perfectly valid, but for
practical purposes far in advance of the time. Their application
demanded a knowledge of stellar light-gradations, which, even now, has
been only partially attained. His surprising anticipation of this mode
of inquiry came, therefore, to nothing.

His device of “limiting apertures” was a simultaneous invention. It
was designed as a measure of relative star-distances. Pointing two
similar telescopes upon two unequal stars, he equalised them to the
eye by stopping down the aperture of the instrument directed towards
the brighter object. Assuming each to emit the same quantity of light,
their respective distances would then be inversely as the diameters of
the reflecting surfaces by which they were brought to the same level of
apparent lustre. But the enormous real diversities of stellar size and
brightness render this plan of action wholly illusory. Even for average
estimates, proper motion is apparently a safer criterion of distance
than magnitude.

Herschel employed the method of apertures with better success to
ascertain the comparative extent of natural and telescopic vision. The
boundary of the former was placed at “the twelfth order of distance.”
Sirius, that is to say, removed to twelve times its actual remoteness,
would be a barely discernible object to the naked eye. The same star
carried seventy-five times further away still, could be seen as a faint
light-speck with his twenty-foot telescope; and, transported 192 times
beyond the visual limit, would make a similar appearance in the field
of the forty-foot. These figures, multiplied by twelve, represented,
in his expressive phrase, the “space-penetrating power” of his
instruments. Their range extended respectively to 900 and 2,300 times
the distance of his “standard star.” He estimated, moreover, that,
through the agency of the larger, light might become sensible to the
eye after a journey lasting nearly seven thousand years! So that, as he
said, his telescopes penetrated both time and space.

His last observation of the Milky Way showed it to be in parts
“fathomless,” even with the forty-foot. No sky-background could be
seen, but only the dim glow of “star-dust.” This effect he attributed
to the immeasurable extension, in those directions, of the stellar
system. The serried orbs composing it, as they lay further and further
from the eye, became at last separately indistinguishable. Herschel, as
has been said, formulated no second theory of galactic structure after
that of 1784–5 had been given up. What he thought on the subject, with
ripened experience for his guide, can only be gathered piecemeal from
his various writings. The general appearance of

      That “broad and ample road, whose dust is gold,
      And pavement stars,”

he described as “that of a zone surrounding our situation in the
solar system, in the shape of a succession of differently condensed
patches of brightness, intermixed with others of a fainter tinge.”
And he evidently considered this _seeming_ to be in fair accord with
reality. The “patches of brightness” stood for genuine clusters,
incipient, visibly forming, or formed. They are made up of stars not
less lustrous, but much more closely collected than Sirius, Arcturus,
or Capella. The smallness of galactic stars would thus be an effect
of distance, while their crowding is a physical fact. The whole of
these clusters are (on Herschel’s view) aggregated into an irregular,
branching ring, distinct from, although bound together into one system
with the brilliants of the constellations. “Our sun,” he emphatically
affirmed in 1817, “with all the stars we can see with the eye, are
deeply immersed in the Milky Way, and form a component part of it.”

He took leave of the subject which had engrossed so many of his
thoughts in a paper read before the Royal Society, June 11th, 1818.
In it he showed how the “equalising” principle could be applied to
determine the relative distances of “globular and other clusters,”
provided only that their component stars are of the rank of Sirius.
It is improbable, however, that this condition is fulfilled. In open
groups, such as the Pleiades, enormous suns are most likely connected
with minute self-luminous bodies; but the stars compressed into
“globular clusters” appear to be more uniform, and may, perhaps, be
intermediate in magnitude. Yet here again, the only thing certain is
the prevalence of endless variety. Celestial systems are not turned out
by the dozen, like articles from a factory. Each differs from the rest
in scale, in structure, in mechanism. Attempts to reduce all to any
common standard must then prove futile. Disparities of distance are of
course concerned in producing their varieties of aspect, coarse-looking
“balls of stars” being, necessarily, on the whole, less remote than
those of smoother texture. Finer graining, however, may also be due to
a composition out of smaller and closer masses. The two causes concur,
and the share of each in producing a certain effect cannot, in any
individual case, be apportioned.

Herschel was indeed far too philosophical to adopt rigid lines of
argument. His reasoning did not extend “so far as to exclude a
real difference, not only in the size, but also in the number and
arrangement of the stars in different clusters.” Nevertheless,
the discussion founded upon it is no longer convincing. To modern
astronomers it appears to travel quite wide of the mark. Its interest
consists in the proof given by it that the problem of sidereal
distances, the original incentive to Herschel’s reviews of the
heavens, attracted his attention to the very end of his thinking life.
Throughout his long career, the profundities of the universe haunted
him. He sought, _per fas, per nefas_, trustworthy measures of the
“third dimension” of celestial space. The object of his search was out
of reach, and has not even now been fully attained; but the path it led
him by was strewn with discoveries.

The nets spread in his “sweeps” brought in, besides double stars,
plentiful takes of the filmy objects called “nebulæ.” He recognised
with amazement their profusion in certain tracts of the sky; increased
telescopic light-grasp never failed to render a further supply visible;
the heavens teemed with them. He presented a catalogue of 1,000 to the
Royal Society in 1786, a second equally comprehensive in 1789, and a
supplementary list of 500 in 1802. Their natural history fascinated
him. What they were, what they had been, and what they should come to,
formed the subject of many of those ardent meditations which supplied
motive power for his researches. He not only laid the foundation of
nebular science, but carried the edifice to a considerable height,
distinguishing the varieties of its objects, and classifying them
according to their gradations of brightness. Some presented a most
fantastic appearance.

“I have seen,” he wrote in 1784, “double and treble nebulæ variously
arranged; large ones with small, seeming attendants; narrow, but much
extended lucid nebulæ or bright dashes; some of the shape of a fan,
resembling an electric brush, issuing from a lucid point; others of
the cometic shape, with a seeming nucleus in the centre, or like
cloudy stars surrounded with a nebulous atmosphere; a different sort,
again, contained a nebulosity of the milky kind, like that wonderful,
inexplicable phenomenon about Theta Orionis; while others shine with a
fainter mottled kind of light which denotes their being resolvable into
stars.”

He, “through the mystic dome,” discerned

     “Regions of lucid matter taking form,
        Brushes of fire, hazy gleams,
      Clusters and beds of worlds, and bee-like swarms
        Of suns and starry streams.”

Annular and planetary nebulæ were _as such_, first described by him.
“Among the curiosities of the heavens,” he announced in 1785, “should
be placed a nebula that has a regular concentric dark spot in the
middle, and is probably a ring of stars.” This was the famous annular
nebula in Lyra, then a unique specimen, now the type of a class.

The planetary kind, so-called from their planet-like discs, were
always more or less of an enigma to him. The vividness and uniformity
of their light appeared to cut them off from true nebulæ; on mature
consideration, he felt driven to suppose them “compressed star-groups.”
“If it were not, perhaps, too hazardous,” he went on, “to pursue
a former surmise of a renewal in what I figuratively called the
laboratories of the universe, the stars forming these extraordinary
nebulæ, by some decay or waste of nature, being no longer fit for their
former purposes, and having their projectile forces, if any such they
had, retarded in each other’s atmospheres, rush at last together, and
either in succession, or by one general tremendous shock, unite into a
new body. Perhaps the extraordinary and sudden blaze of a new star in
Cassiopeia’s Chair, in 1572, might possibly be of such a nature.”

At that early stage of his inquiries, Herschel regarded all nebulæ
indiscriminately as composed of genuine stars. It was almost inevitable
that he should do so. For each gain in telescopic power had the effect
of transferring no insignificant proportion of them from the nebular
to the stellar order. There was no apparent reason for drawing a line
anywhere. The inference seemed irresistible, that resolvability was
simply a question of optical improvement. As Messier’s _nébuleuses sans
étoiles_ had yielded to Herschel’s telescopes, so--it might fairly
be anticipated--the “milky” streaks and patches seen by Herschel
would curdle into stars under the compulsion of the still mightier
instruments of the future. He was led on--to use his own expressions
in 1791--“by almost imperceptible degrees from evident clusters,
such as the Pleiades, to spots without a trace of stellar formation,
the gradations being so well connected as to leave no doubt that all
these phenomena were equally stellar.” They were what Lambert and Kant
had supposed them to be--island-universes, vast congeries of suns,
independently organised, and of galactic rank. They were, each and all,
glorious systems, barely escaping total submergence in the illimitable
ocean of space. Under the influence of these grandiose ideas, Herschel
told Miss Burney, in 1786, that with his “large twenty-foot” he had
“discovered 1,500 universes!” Fifteen hundred “whole sidereal systems,
some of which might well outvie our Milky Way in grandeur.”

His contemplations of the heavens showed him everywhere traces of
progress--of progress rising towards perfection, then sinking into
decay, though with a sure prospect of renovation. He was thus led to
arrange the nebulæ in a presumed order of development. The signs of
interior condensation traceable in nearly all, he attributed to the
persistent action of central forces. Condensation, then, gave evidence
of age. Aggregated stars drew closer and closer together with time. So
that scattered or branching formations were to be regarded as at an
early stage of systemic existence; globular clusters, as representing
universes still in the prime of life; while objects of the planetary
kind were set down as “very aged, and drawing on towards a period of
change, or dissolution.”

Our own nebula he characterised as “a very extensive, branching
congeries of many millions of stars,” bearing upon it “fewer marks of
profound antiquity than the rest.” Yet, in certain regions, he found
“reason to believe that the stars are now drawing towards various
secondary centres, and will in time separate into different clusters.”
As an example of the ravages of time upon the galactic structure,
he adverted to a black opening, four degrees wide, in the Zodiacal
Scorpion, bordered on the west by an exceedingly compact cluster
(Messier’s No. 80), possibly formed, he thought, of stars drawn from
the adjacent vacancy. The chasm was to him one of the most impressive
of celestial phenomena. His sister preserved an indelible recollection
of hearing him, in the course of his observations, after a long, awful
silence, exclaim, “Hier ist wahrhaftig ein Loch im Himmel!” (Here,
truly, is a hole in the sky); and he recurred to its examination
night after night and year after year, without ever clearing up, to
his complete satisfaction, the mystery of its origin. The cluster
significantly located at its edge was lit up in 1860 by the outburst of
a temporary star.

This was not the sole instance noted by Herschel of the conjunction
of a chasm with a cluster; and chasms and clusters alike told the
same story of dilapidation. He foresaw, accordingly, as inevitable,
the eventual “breaking-up” of the Milky Way into many small, but
independent nebulæ. “The state into which the incessant action of the
clustering power has brought it at present,” he wrote in 1814, “is a
kind of chronometer that may be used to measure the time of its past
and future existence; and although we do not know the rate of going of
this mysterious chronometer, it is, nevertheless, certain that since
the breaking up of the Milky Way affords a proof that it cannot last
for ever, it equally bears witness that its past duration cannot be
admitted to be infinite.”

Thus the idea of estimating the relative “ages” of celestial
objects--of arranging them according to their progress in development,
originated with Herschel in 1789. “This method of viewing the heavens,”
he added, “seems to throw them into a new kind of light. They are
now seen to resemble a luxuriant garden which contains the greatest
variety of productions in different flourishing beds; and one
advantage we may at least reap from it is that we can, as it were,
extend the range of our experience to an immense duration. For, is
it not almost the same thing whether we live successively to witness
the germination, blooming, foliage, fecundity, fading, withering, and
corruption of a plant, or whether a vast number of specimens, selected
from every stage through which the plant passes in the course of its
existence, be brought at once to our view?”

But while he followed the line of continuity thus vividly traced,
another crossing, and more or less interfering with it, opened out
before him. The discovery of a star in Taurus, “surrounded with a
faintly luminous atmosphere,” led him, in 1791, to revise his previous
opinions regarding the nature of nebulæ. He was not at all ashamed of
this fresh start. No fear of “committing himself” deterred him from
imparting the thoughts that accompanied his multudinous observations.
He felt committed to nothing but truth. He was advancing into an
untrodden country. At every step he came upon unexpected points of
view. The bugbear of inconsistency could not prevent him from taking
advantage of each in turn to gain a wider prospect.

Until 1791 Herschel never doubted that gradations of distance fully
accounted for gradations of nebular resolvability. He had been led on,
he explained, by almost imperceptible degrees from evident clusters
to spots without a trace of stellar formation, no break anywhere
suggesting the possibility of a radical difference of constitution.
“When I pursued these researches,” he went on, “I was in the situation
of a natural philosopher who follows the various species of animals
and insects from the height of their perfection down to the lowest ebb
of life; when, arriving at the vegetable kingdom, he can scarcely point
out to us the precise boundary where the animal ceases and the plant
begins; and may even go so far as to suspect them not to be essentially
different. But, recollecting himself, he compares, for instance,
one of the human species to a tree, and all doubt upon the subject
vanishes. In the same manner we pass by gentle steps from a coarse
cluster to an object such as the nebula in Orion, where we are still
inclined to remain in the once adopted idea of stars exceedingly remote
and inconceivably crowded, as being the occasion of that remarkable
appearance. It seems, therefore, to require a more dissimilar object
to set us right again. A glance like that of the naturalist, who casts
his eye from the perfect animal to the perfect vegetable, is wanting
to remove the veil from the mind of the astronomer. The object I have
mentioned above is the phenomenon that was wanting. View, for instance,
the nineteenth cluster of my sixth class, and afterwards cast your eye
on this cloudy star, and the result will be no less decisive than that
of the naturalist. Our judgment, I venture to say, will be that _the
nebulosity about the star is not of a starry nature_.”

In this manner he inferred the existence of real nebulous matter--of
a “shining fluid” of unknown and unimaginable properties. Was it
perhaps, he asked himself, a display of electrical illumination, like
the aurora borealis, or did it rather resemble the “magnificent cone of
the zodiacal light?” A boundless field of speculation was thrown open.
“These nebulous stars,” he added, “may serve as a clue to unravel
other mysterious phenomena.”

As their close allies, he now recognised planetary nebulæ, the
“milkiness, or soft tint of their light,” agreeing much better with the
supposition of a fluid, than of a stellar condition. And he rightly
placed in the same category the Orion nebula, and certain “diffused
nebulosities” which he had observed just to tarnish the sky over wide
areas. These last might, he considered, be quite near the earth, and
the object in Orion not more distant than perhaps an average second
magnitude star.

The relations of the sidereal to the nebular “principle” exercised
Herschel’s thoughts during many years. He had no sooner reasoned out
the existence in interstellar space of a rarefied, self-luminous
substance, than he began to interrogate himself as to its probable
function. Nature was to him the expression of Supreme Reason. He could
only conceive of her doings as directed towards an intelligible end.
Hence his confidence that rational investigation must lead to truth.

Already in 1791 he hinted at the conclusion which he foresaw. The
envelope of a “cloudy star” was, he declared, “more fit to produce
a star by its condensation than to depend upon the star for its
existence.” And the surmise was confirmed by his detection, in a
planetary nebula, of a sharp nucleus, or “generating star,” possibly to
be completed in time by the further accumulation of luminous matter.

His conjectures developed in 1811 into a formal theory. The cosmical
fluid was met with in all stages of condensation. Nebulous tracts of
almost evanescent lustre were connected in an unbroken series with
slightly “burred” objects, wanting only a few last touches to make them
finished stars. The extremes, as he said, had been, by his “critical
examination of the nebulous system,” “connected by such nearly allied
intermediate steps, as will make it highly probable that every
succeeding state of the nebulous matter is the result of the action of
gravitation upon it while in a foregoing one.”

In 1814 he traced the progress towards maturity of binary systems.
Originating in double nebulæ incompletely dissevered--Siamese-twin
objects, of which he had collected 139 examples--they next appeared
as nebulously-connected stars, finally as a pair materially isolated,
and linked together by the sole tie of gravitation. Scattered clusters
represented, in his scheme of celestial progress, a state antecedent
to that of globular clusters. “The still remaining irregularity of
their arrangement,” he said, “additionally proves that the action of
the clustering power has not been exerted long enough to produce a more
artificial construction.” He made, too, the important admission that
clusters apparently “in, or very near the Milky Way,” were truly part
and parcel of that complex agglomeration.

But what of his “fifteen hundred universes,” which had now logically
ceased to exist? The stellar and nebular “principles” had virtually
coalesced; both were included in the galactic system. The question
of “island universes” was accordingly left in abeyance; although
Herschel certainly believed in 1818 that among the multitude of
“ambiguous objects”--we should call them irresolvable nebulæ--many
exterior firmaments were included. Yet what he had ascertained about
the distribution of nebulæ should alone have sufficed to shatter this
remnant of a conviction.

The fact became clear to him during the progress of his “sweeps” that
nebulæ, to some extent, _replace stars_. He found them to occur in
“parcels,” more or less embedded with stars, “beds” and “parcels”
together being surrounded by blank spaces. This arrangement grew so
familiar to him that he used to notify his assistant, when stars
thinned out in the zone he was traversing, “to prepare for nebulæ.”
A wider relationship, brought within view by the large scale of
his labours, was defined by his fortunate habit of charting, for
convenience of identification, each newly-discovered batch of nebulæ.

“A very remarkable circumstance,” he wrote in 1784, “attending the
nebulæ and clusters of stars, is that they are arranged into strata,
which seem to run on to a great length; and some of them I have already
been able to pursue, so as to guess pretty well at their form and
direction. It is probable enough that they may surround the whole
apparent sphere of the heavens, not unlike the Milky Way.”

In the following year he spoke no longer of a zone, but of two vast
groupings of nebulæ about the opposite poles of the Milky Way. That
is to say, where stars are scarcest nebulæ are most abundant. The
correspondence did not escape him; but he did not recognise its
architectonic meaning. He had traced out the main plan of the stellar
world; he had discovered, not merely thousands of nebulæ, but the
nebular system; he had shown that stars and nebulæ were intimately
associated; he had even made it clear that nebular distribution was
governed by the lines of galactic structure. It only remained to draw
the obvious inference that these related parts made up one whole--that
no more than a single universe is laid open to human contemplation.
This was done by Whewell thirty years after his death.




CHAPTER IV.

HERSCHEL’S SPECIAL INVESTIGATIONS.


Double stars were, when Herschel began to pay attention to them,
regarded as mere chance productions. No suspicion was entertained
that a real, physical bond united their components. Only the Jesuit
astronomer, Christian Mayer, maintained that bright stars were often
attended by faint ones; and since his observations were not such as
to inspire much confidence, his assertions counted for very little.
“In my opinion,” Herschel wrote in 1782, “it is much too soon to form
any theories of small stars revolving round large ones.” He, indeed,
probably even then, suspected that close _equal_ stars formed genuine
couples; but he waited, if so, for evidence of the connection. The
chief subject of his experiments on parallax was Epsilon Boötis, an
exquisitely tinted, unequal pair. But he soon became aware that either
stellar parallax was elusively small, or that he was on the wrong track
for detecting it. And, since his favourite stars have proved to be a
binary combination, it was, of course, drawing water in a sieve to make
one the test of perspective shifting in the other.

The number of Herschel’s double stars alone showed them to be integral
parts of an express design. Such a crop of casualties was out of all
reasonable question. And it was actually pointed out in 1784 by John
Michell, a man of extraordinary sagacity, that the odds in favour of
their physical union were truly “beyond arithmetic.”

Herschel meantime kept them under watch and ward, and after the lapse
of a score of years found himself in a position to speak decisively.
On July 1, 1802, he informed the Royal Society that “casual situations
will not account for the multiplied phenomena of double stars,” adding,
“I shall soon communicate a series of observations proving that many
of them have already changed their situation in a progressive course,
denoting a periodical revolution round each other.” A year later he
amply fulfilled this pledge. Discussing in detail the displacements
brought to light by his patient measurements, he made it clear that
they could be accounted for only by supposing the six couples in
question to be “real binary combinations, intimately held together
by the bond of mutual attraction.” His conclusion was, in each case,
ratified by subsequent observation. The stars instanced by him--Castor,
Gamma Leonis, Epsilon Boötis, Delta Serpentis, Gamma Virginis, and
Zeta Herculis--are all noted binaries. Not satisfied with establishing
the fact, Herschel assigned the periods of their revolutions. But he
could only do so on the hypothesis of circular motion, while the real
orbits are highly elliptical. His estimates then went necessarily wide
of the mark. For one pair only, he was able to use an observation
anterior to his own. Bradley had roughly fixed, in 1759, the relative
position of the components of Castor, the finest double star in the
northern heavens; and the preservation of the record in Dr. Maskelyne’s
note-book extended by twenty years the basis of Herschel’s conclusions
regarding this system.

He continued, in 1803, his discussions of double stars; announced
a leisurely circulation of both the pairs composing the typical
“double-double star,” Epsilon Lyræ; and conjectured the union of the
two into one grand whole--a forecast verified by the evidence of
common proper motion. The Annus Magnus of the quadruple system cannot,
according to Flammarion, be less than a million of years.

The discovery of binary stars was, in Arago’s phrase, “one with a
future.” In itself an amazing revelation, it marked the beginning of
a series of investigations of immense variety and importance. By it,
a science of sidereal mechanics was shown to be possible; the sway of
gravitation received an unlimited extension; and the perception of
order, which is the precursor of knowledge, ranged at once over the
whole visible creation. Herschel, it is true, had not the means of
formally proving that stellar orbits are described in obedience to the
Newtonian law. His affirmative assertion rested only on the analogy of
the solar system. But the rightness of his judgment has never seriously
been called in question.

His research into the transport of the solar system through space
proved, as Bessel said, that the activity of his mind was independent
of the stimulus supplied by his own observations. It was one of his
most brilliant performances.

The detection of progressive star-movements was due to Halley. It
was announced in 1718. The bright objects spangling the sky are then
“fixed” only in name. “But if the proper motion of the stars be
admitted,” asked Herschel, “who can deny that of our sun?” The same
idea had occurred to several earlier astronomers, but only one, Tobias
Mayer, of Göttingen, had tried to test it practically; and he had
failed. “To discern the proper motion of the sun between so many other
motions of the stars,” Herschel might well designate “an arduous task.”
Yet it was not on that account to be neglected. The conditions of the
problem were perfectly clear to him. If the sun alone were in motion,
the stars should unanimously appear to drift backward from the “apex,”
or point on the sphere towards which his journey was directed. The
heavens would open out in front of his advance, and close up behind.
The effect was compared by Mayer to the widening prospect and narrowing
vista of trees to a man walking through a forest. On this supposition,
the perspective displacements of any two stars sufficiently far apart
in the sky would suffice to determine the solar apex. For it should
coincide with the intersection of the two great circles continuing the
directions of those displacements. But the question is far from being
of this elementary nature. The stars are all flitting about on their
own account, after--to our apprehension--a haphazard fashion. The sole
element of general congruity traceable among them is that “systematic,
or higher, parallax,” by which each of them is, according to a
determinate proportion, inevitably affected. If this can be elicited,
the line of the sun’s progress becomes at once known.

Herschel treated the subject in the simplest possible manner. Striking
a balance between the proper motions of only seven stars, he deduced,
in 1783, from simple geometrical considerations, an apex for the sun’s
way, marked by the star Lambda Herculis. But while he seemed to proceed
by rule, he was really led by the unerring instinct of genius. His
mode of conducting an investigation, small in compass, yet almost
inconceivably grand in import, distances praise. Its directness and
apparent artlessness strike us dumb with wonder. Eminently suited to
the materials at his command, it was summary, yet, within fairly narrow
limits, secure. And the result has stood the test of time. It ranks,
even now, as a valuable approximation to the truth. He himself regarded
his essay as nothing more than an experimental effort. In a letter to
Dr. Wilson, of Glasgow, he expressed his apprehensions lest his paper
on the sun’s motion “might be too much out of the way to deserve the
notice of astronomers.”

Provided with Maskelyne’s table of thirty-six proper motions, he
resumed the subject in 1805. He now employed a graphical method,
drawing great circles to represent the observed stellar movements, and
planting his apex impartially in the midst of their intersections. It
was, however, less happily located than that of 1783. The constellation
Hercules again just included it; but it lay certainly too far west,
and probably too far north. The memoir conveying the upshot of the
research is, none the less, a masterpiece. Philosophy and common-sense
have rarely been so fortunately blended as in this discussion. Without
any mathematical apparatus, the plan of attack upon a recondite problem
is expounded with the utmost generality and precision. The reasoning
is strong and sure; intelligible to the ignorant, instructive to the
learned.

In his earlier paper, Herschel, while venturing only to “offer a few
distant hints” as to the _rate_ of the sun’s travelling, expressed
the opinion that it could “certainly not be less than that which the
earth has in her annual orbit.” That is to say, his minimum estimate
was then nineteen miles per second. A direct inquiry, on the other
hand, convinced him, in 1806, that the solar motion, viewed at right
angles from the distance of Sirius, would cover yearly an arc of
1″. 112. This he called “its quantity;” the corresponding velocity
remained undetermined. We can, however, now, since the real distance
of his assumed station has been determined, translate this angular
value into a linear speed of about nine miles a second. The mean of
his two estimates, or fourteen miles a second, probably differs little
from the actual rate at which the solar system is being borne to its
unimaginable destination.

His conclusions regarding the solar translation obtained little notice,
and less acceptance from his contemporaries and immediate successors.
His son rejected them as untrustworthy; Bessel, the greatest authority
of his time in the science of “how the heavens move,” declared in
1818 that the sun’s apex might be situated in any other part of the
sky with as much probability as in the constellation Hercules. Not
until Argelander, by a strict treatment of multiplied and improved
data, arrived in 1837 at practically the same result, did Herschel’s
anticipatory efforts obtain the recognition they deserved. Scarcely in
any department has there been put on record so well-directed a leap
into the dark of coming discovery.

The systematic light-measurement of the stars began with the same
untiring investigator. He described in 1796 the method since named
that of “sequences,” and presented to the Royal Society the first of
six Photometric Catalogues embracing nearly all the 2,935 stars in
Flamsteed’s “British Catalogue.” They gave comparative brightnesses
estimated with the naked eye; classification by magnitudes was put
aside as vague and misleading. The “sequences” serving for their
construction were lists of stars arranged, by repeated trials, in
order of lustre, and rendered mutually comparable by the inclusion
in each of a few members of the preceding series. Their combination
into a catalogue was then easily effected. “Simple as my method is in
principle,” he remarked, “it is very laborious in its progress.” On a
restricted scale it is still employed for following the gradations of
change in variable stars.

These researches lay, as Professor Holden expresses it, “directly on
the line of Herschel’s main work.” The separation of the stars into
light-ranks intimates at once something as to their distribution in
space; but the intimations may prove deceptive unless the divisions be
accurately established. Hence, stellar photometry is an indispensable
adjunct to the study of sidereal construction. Herschel prosecuted
the subject besides with a view to ascertaining the constancy of
stellar lustre. He had been struck with singular discordances between
magnitudes assigned at different dates. Not to mention stars obviously
variable, there were others which seemed to be affected by a slow,
secular waxing or waning. In some of the instances alleged by him,
the alteration was no doubt fictitious--a record of antique errors;
but there was a genuine residuum. Thus, the immemorially observed
constituents of the Plough preserve no fixed order of relative
brilliancy, now one, now another of the septett having, at sundry
epochs, assumed the primacy; while a small star in the same group,
Alcor, the “rider” of the second “horse,” has, in the course of a
millennium, plainly thrown off some part of its former obscurity. The
Arabs in the desert regarded it as a test of penetrating vision; and
they were accustomed to oppose “Suhel” to “Suha” (Canopus to Alcor) as
occupying respectively the highest and lowest posts in the celestial
hierarchy. So that _Vidit Alcor, at non lunam plenam_, came to be a
proverbial description of one keenly alive to trifles, but dull of
apprehension for broad facts. Now, however, Alcor is an easy naked-eye
object. One needs not be a “tailor of Breslau,” or a Siberian savage,
to see it. The little star is unmistakably more luminous than of old.

An inversion of brilliancy between Castor and Pollux, and between the
two leading stars in the Whale, is further generally admitted to have
taken place during the eighteenth century. The prevalence of such
vicissitudes was deeply impressive to Herschel, especially through
their bearing upon the past and future history of our own planet.
“If,” he said, “the similarity of stars with our sun be admitted, how
necessary will it be to take notice of the fate of our neighbouring
_suns_, in order to guess at that of our own. The _star_ which we have
dignified by the name of _Sun_ may to-morrow begin to undergo a gradual
decay of brightness, like Alpha Ceti, Alpha Draconis, Delta Ursæ
Majoris, and many other diminishing stars. It may suddenly increase
like the wonderful star in Cassiopeia, or gradually come on like
Pollux, Beta Ceti, etc. And, lastly, it may turn into a periodical one
of twenty-five days’ duration (the solar period of rotation), as Algol
is one of three days, Delta Cephei of five days, etc.” He found it,
accordingly, “perhaps the easiest way of accounting for past changes
in climate to surmise that our sun has been formerly sometimes more,
sometimes less, bright than it is at present.” Herschel attempted,
in 1798, to analyse star-colours by means of a prism applied to the
eye-glasses of his reflector. Nothing of moment could at that time come
of such experiments; but they deserve to be remembered as a sort of
premonition of future methods of research into the physical condition
of the stars.

His attention to the sun might have been exclusive, so diligent was
his scrutiny of its shining surface. Many of its peculiarities were
first described by him, and none escaped him, except the “deeper
deep,” or black nucleus of spots, detected by Dawes in 1852. The dusky
“pores” and brilliant “nodules,” the corrugations, indentations, and
ridges; the manifold aspects of spots, or “openings;” their “luminous
shelving sides,” known as penumbræ; were all noted in detail, ranged in
proper order, and studied in their mutual relations. Spots presented
themselves to him as evident depressions in the luminous disc; faculæ,
“so far from resembling torches,” appeared “like the shrivelled
elevations upon a dried apple, extended in length, and most of them
joined together, making waves, or waving lines.” Towards the north and
south, he went on, “I see no faculæ; there is all over the sun a great
unevenness, which has the appearance of a mixture of small points of
an unequal light; but they are evidently a roughness of high and low
parts.”

His theory of the solar constitution was a development of Wilson’s.
It was clearly conceived, firmly held, and boldly put forward. The
definite picturesqueness, moreover, of the language in which it was
clothed, at once laid hold of the public imagination, and gave it
a place in public favour from which it was dislodged only by the
irresistible assaults of spectrum analysis.

The sun was regarded by Herschel as a cool dark body surrounded by
an extensive atmosphere made up of various elastic fluids. Its upper
stratum--Schröter named it the “photosphere”--was of cloud-like
composition, and consisted of lucid matter precipitated from the
elastic medium by which it was sustained. Its depth was estimated at
two or three thousand miles, and the nature of its emissions suggested
a comparison with the densest coruscations of the aurora borealis.
Below lay a region of “planetary,” or protective clouds. Dense, opaque,
and highly reflective, “they must add,” he said, “a most capital
support to the splendour of the sun by throwing back so great a share
of the brightness coming to them.” Their movements betrayed the action
of vehement winds; and indeed the continual “luminous decompositions”
producing the radiating shell, with the consequent regeneration of
atmospheric gases beneath, “must unavoidably be attended with great
agitations, such as with us might even be called hurricanes.” The
formation and ascent of “empyreal gas” would cause, when moderate in
quantity, pores, or small openings in the brilliant layers. But should
it happen to be generated in uncommon quantities, “it will burst
through the planetary regions of clouds, and thus will produce great
openings; then, spreading itself above them, it will occasion large
shallows, and, mixing afterwards gradually with other superior gases,
it will promote the increase, and assist in the maintenance of the
general luminous phenomena.”

The solid globe thus girt round with cloud and fire was depicted as
a highly eligible place of residence. An equable climate, romantic
scenery, luxuriant vegetation, smiling landscapes, were to be found
there. It might, accordingly, be admitted without hesitation that “the
sun was richly stored with inhabitants.” For the lucid shell visible
from the exterior possessed, according to this theory, none of the
all-consuming ardour now attributed to it. Its blaze was a superficial
display; beneath, “the immense curtain of the planetary clouds was
everywhere closely drawn” round a world perfectly accommodated to vital
needs.

In order to reconcile this supposed state of things with the observed
order of nature, it was suggested that traces of it subsist in the
planets, “all of which, we have pretty good reason to believe, emit
light in some degree.” The night-side illumination of Venus, the
sinister glare of the eclipsed moon, the auroral glimmerings of the
earth, were adduced as evidence to this effect. The contrast between
the central body and its dependants was softened down to the utmost.

“The sun, viewed in this light,” Herschel wrote in 1794, “appears to be
nothing else than a very eminent, large, and lucid planet, evidently
the first, or, in strictness of speaking, the only primary one of our
system; all others being truly secondary to it. Its similarity to the
other globes of the solar system with regard to its solidity, its
atmosphere, and its diversified surface; the rotation upon its axis,
and the fall of heavy bodies, lead us on to suppose that it is also
most probably inhabited, like the rest of the planets, by beings whose
organs are adapted to the peculiar circumstances of that vast globe.”

To us, nearing the grey dawn of the twentieth century, the idea seems
extravagant; it was, in the eighteenth, plausible and alluring. The
philosophers of that age regarded the multiplicity of inhabited
worlds as of axiomatic certainty. The widest possible diffusion of
life followed, they held, as a corollary from the beneficence of the
Creator; while their sense of economy rendered them intolerant of
_wasted_ globes. Herschel was then reluctant to attribute to the sun
a purely _altruistic_ existence. Only from the point of view of our
small terrestrial egotism could so glorious a body figure as solely
an attractive centre, and a focus of warmth and illumination to a
group of planets. Besides, looking abroad through the universe, we see
multitudes of stars which can exercise no ministerial functions. Those
united to form compressed clusters, or simply joined in pairs, are
unlikely, it was argued, to carry a train of satellites with them in
their complex circlings. Unless, then, “we would make them mere useless
brilliant points,” they must “exist for themselves,” and claim primary
parts in the great cosmical life-drama.

Herschel’s sun is to us moderns a wholly fabulous body. Still, there
is a fantastic magnificence about the conception so strongly realised
by his powerful imagination. Moreover, its scientific value was by
no means inconsiderable. It represented the first serious effort to
co-ordinate solar phenomena; it implied the spontaneous action of some
sort of machinery for the production of light and heat. Spots were
associated with a circulatory process; the photosphere was portrayed
under its true aspect. The persistence of its hollows and heights, its
pores and rugosities, convinced Herschel that the lustrous substance
composing it was “neither a liquid nor an elastic fluid,” which should
at once subside into an unbroken level. “It exists, therefore,” he
inferred, “in the manner of lucid clouds swimming in the transparent
atmosphere of the sun.”

“The influence of this eminent body on the globe we inhabit,” he wrote,
continuing the subject in 1801, “is so great, and so widely diffused,
that it becomes almost a duty to study the operations which are carried
on upon the solar surface.” This duty he fulfilled to perfection. His
telescopic readings from the changeful solar disc were of extraordinary
precision and comprehensiveness. They show his powers as an observer
perhaps at their best. And, since reasoning was with him inseparable
from seeing, the appearances he noted took, as if of their own accord,
their proper places. The history of spots was completely traced. He
recorded their birth by the enlargement of pores; their development
and sub-division; established their connexion with faculous matter,
piled up beside them like mountain-ranges round an Alpine lake, or
flung across their cavities like blazing suspension-bridges; and
watched finally their closing-up and effacement, not even omitting the
post-mortem examination of the disturbances they left behind.

One of Herschel’s curiously original enterprises was his attempt to
ascertain a possible connexion between solar and terrestrial physics.
“I am now much inclined to believe,” he stated in 1801, “that openings
with great shallows, ridges, nodules, and corrugations, may lead us to
expect a copious emission of heat, and, therefore, mild seasons. And
that, on the contrary, pores, small indentations, and a poor appearance
of the luminous clouds, the absence of ridges and nodules, and of
large openings and shallows, will denote a spare emission of heat,
and may induce us to expect severe seasons. A constant observation
of the sun with this view, and a proper information respecting the
general mildness or severity of the seasons in all parts of the world,
may bring this theory to perfection, or refute it, if it be not well
founded.”

But the available data regarding weather-changes turning out to be
exceedingly defective, he had recourse to the celebrated expedient of
comparing the state of the sun in past years with the recorded prices
of corn. Fully admitting the inadequacy of the criterion, he still
thought that the sun being “the ultimate fountain of fertility, the
subject may deserve a short investigation, especially as no other
method is left for our choice.” He obtained, as the upshot, partial
confirmation of the surmise that “some temporary defect of vegetation”
ensued upon the subsidence of solar agitation. In plainer language,
food-stuffs tended to become dear when sun-spots were few and small. No
signs of cyclical change could, however, be made out. The discovery of
the “sun-spot period” was left to Schwabe. This admirable preliminary
effort to elicit the earth’s response to solar vicissitudes was
denounced by Brougham as a “grand absurdity;” and the readers of the
second number of the _Edinburgh Review_ were assured that “since the
publication of ‘Gulliver’s Travels,’ nothing so ridiculous had ever
been offered to the world!”

Herschel did not neglect the planets. His observations of Venus
extended from 1777 to 1793. Their principal object was to ascertain the
circumstances of the planet’s rotation; but they eluded him; which,
considering that they are still quite uncertain, is not surprising.
He would probably have communicated nothing on the subject had he not
been piqued into premature publication by Schröter’s statement that
the mountains of Venus rose to “four, five, or even six times the
perpendicular elevation of Chimborazo.” Herschel did not believe in
them, and expressed his incredulity in somewhat sarcastic terms. “As to
the mountains in Venus,” he wrote, “I may venture to say that no eye
which is not considerably better than mine, or assisted by much better
instruments, will ever get a sight of them.” He rightly inferred,
however, the presence of an extensive atmosphere from the bending of
the sun’s rays so as to form much more than a semicircular rim of light
to the dark disc of the planet when near inferior conjunction--that is,
when approximately in a right line between us and the sun. He fully
ascertained, too, the unreality of the Cytherean phantom-satellite.
The irritability visible in this paper made a solitary exception
to Herschel’s customary geniality. It might have led to a heated
controversy but for the excellent temper of Schröter’s reply.

Although we may not be prepared to gainsay Herschel’s dictum that “the
analogy between Mars and the earth is perhaps by far the greatest in
the whole solar system,” we can hardly hold it to be so probable as he
did that “its inhabitants enjoy a situation in many respects similar
to ours.” Yet the modern epoch in the physical study of Mars began
with his announcement in 1784 that its white polar caps spread and
shrank as winter and summer alternated in their respective hemispheres.
His conclusion of their being produced by snowy depositions from
“a considerable, though moderate, atmosphere,” is not likely to be
overthrown. He established, besides, the general permanence of the dark
markings, notwithstanding minor alterations due, he supposed, to the
variable distribution of clouds and vapours on the planet’s surface.

This vigilant “watcher of the skies” laid before the Royal Society,
May 6th, 1802, his “Observations of the two lately discovered Bodies.”
These were Ceres and Pallas, which, with Juno and Vesta, picked up
shortly afterwards, constituted the vanguard of the planetoid army.
Herschel foresaw its arrival. He adopted unhesitatingly Olbers’s theory
of their disruptive origin, and calculated that Mercury, the least
of the true planets, might be broken up into 35,000 masses no larger
than Pallas. An indefinite number of such fragments (about 420 are
now known) were accordingly inferred to circulate between the orbits
of Mars and Jupiter. He distinguished their peculiarities, and, since
they could with propriety be designated neither planets nor comets, he
proposed for them the name of “asteroids.” But here again he incurred,
to use his own mild phrase, “the illiberal criticism of the _Edinburgh
Review_.” “Dr. Herschel’s passion for coining words and idioms,”
Brougham declared, “has often struck us as a weakness wholly unworthy
of him. The invention of a name is but a poor achievement in him who
has discovered whole worlds.” The reviewer forgot, however, that new
things will not always fit into the framework of old terminology. He
added the contemptible insinuation that Herschel had devised the word
“asteroid” for the express purpose of keeping Piazzi’s and Olbers’s
discoveries on a lower level than his own of Uranus.

Herschel made no direct reply to the attack; only pointing out, in
December, 1804, how aptly the detection of Juno had come to verify his
forecasts. “The specific differences,” he said, “between planets and
asteroids appear now, by the addition of a third individual of the
latter species, to be more fully established; and that circumstance,
in my opinion, has added more to the ornament of our system than the
discovery of another planet could have done.”

His endeavours to determine the diameters of these small bodies were
ineffectual. Although he at first estimated those of Ceres and Pallas
at 162 and 147 miles, he admitted later his inability to decide as to
the reality of the minute discs shown by them; and they were first
genuinely measured by Professor Barnard with the great Lick refractor
in 1894.

The “trade-wind theory” of Jupiter’s belts originated with Herschel;
and he took note of the irregular drifting movements of the spots on
his surface, and their consequent uselessness for determining the
period of his rotation. That of Saturn’s he fixed quite accurately
at ten hours sixteen minutes, with a marginal uncertainty of two
minutes, the period now accepted being of ten hours fourteen minutes.
The possession by this planet of a profound atmosphere was inferred
from the changes in its belts, as well as from some curious phenomena
attending the disappearance of its satellites. They were commonly
seen to “hang on the limb”--that is, to pause during an appreciable
interval on the brink of occultation. Mimas, on one occasion, remained
thus poised during twenty minutes! For so long it was geometrically
concealed, although visible by the effect of refraction. Saturn was
an object of constant solicitude at Slough; and it was only with the
surpassing instruments mounted there that much could be learned about
Galileo’s _altissimo pianeta_. Herschel supposed, with Laplace, the
rings to be solid structures; and he added that the interval of 2,500
miles separating them “must be of considerable service to the planet
in reducing the space that is eclipsed by the shadow of the ring.” The
“crape ring” was _seen_, but not recognised. In one of his drawings it
figures as a dusky belt crossing the body of the planet.

His satellite discoveries proved exceedingly difficult to verify. The
Saturnian pair were lost, after he left them, until his son once more
drew them from obscurity. Regarding the outermost member of the system,
Japetus, discovered by Cassini in 1671, Herschel noticed, in 1792, a
singular circumstance. It was already known to vary in brightness; we
receive from it, in fact, four and a-half times more light at certain
epochs than at others. The novelty consisted in showing that this
variation depended upon the satellite’s situation in its orbit in such
a manner as to leave no doubt that, like our moon, it keeps the same
face always directed inwards towards its primary. So that Japetus was
inferred to turn on its axis in the period of its revolution round
Saturn, that is, in seventy-nine and one-third days.

“From its changes” he “concluded that by far the largest part of its
surface reflects much less light than the rest; and that neither the
darkest nor the brightest side of the satellite is turned towards the
planet, but partly the one and partly the other.”

Guessing at once that our moon and Japetus did not present the
only examples of equality in the times of rotation and revolution,
he continued: “I cannot help reflecting with some pleasure on the
discovery of an analogy which shows that a certain uniform plan is
carried on among the secondaries of our solar system; and we may
conjecture that probably most of the satellites are governed by the
same law, especially if it be founded upon such a construction of their
figure as makes them more ponderous towards their primary planet.”
This very explanation was long afterwards adopted by Hansen. The
peculiarity in question may without hesitation be set down as an effect
of primordial tides.

In 1797 Herschel brought forward detailed evidence to shew that his
generalisation applied to the Jovian system; but recent observations at
Lick and Arequipa demand a suspension of judgment on the point.

The Uranian train of attendants was left by Herschel in an unsettled
condition. Two of them, as we have seen, he discovered in 1787; and
he subsequently caught glimpses of what he took to be four others.
But only Oberon and Titania have maintained their status; the four
companions assigned to them are non-existent. An unmistakable interior
pair--Ariel and Umbriel--was, however, discovered by Mr. Lassell, at
Malta, in 1851; and they may possibly have combined with deceptive
star-points to produce Herschel’s dubious quartette. He described in
1798 the exceptional arrangement of the Uranian system. Its circulation
is retrograde. The bodies composing it move from east to west, but in
orbits so tilted as to deviate but slightly from perpendicularity to
the plane of the ecliptic.

No trifling sensation was created in 1783, and again in 1787, by the
news that Herschel had seen three lunar volcanoes in violent eruption.
“The appearance of the actual fire” in one of them was compared by him
to “a small piece of burning charcoal when it is covered with a very
thin coating of white ashes. All the adjacent parts of the volcanic
mountain seemed to be faintly illuminated by the eruption, and were
gradually more obscure as they lay at a greater distance from the
crater.” He eventually became aware that his senses had imposed upon
him; but the illusion was very complete and has since occasionally been
repeated. What was really seen was probably the vivid reflection of
earth-shine from some unusually white lunar summits.

He never knowingly discovered a comet, although some few such bodies
possibly ensconced themselves, under false pretences, in his lists
of nebulæ. But he made valuable observations upon the chief of those
visible in his time, and introduced the useful terms, corresponding to
instructive distinctions, “head,” “nucleus,” and “coma.” He inferred
from the partial phases of the comet of 1807, that it was in a measure
self-luminous; and from their total absence in the great comet of 1811,
that its light was almost wholly original. The head of this object,
which shone with an even, planetary radiance, he determined to be
127,000, the star-like nucleus within, 428 miles across. The tail he
described as “a hollow, inverted cone,” one hundred millions of miles
long, and fifteen millions broad. This prodigious appurtenance was,
in grade of luminosity, an exact match for the Milky Way. That comets
wear out by the waste of their substance at perihelion, he thought
very probable; the extent of their gleaming appendages thus serving
as a criterion of their antiquity. They might, indeed, arrive in the
solar system already shorn of much of their splendour by passages round
other suns than ours; but their “age” could, in any case, be estimated
according to the progress made in their decline from a purely nebulous
to an almost “planetary” state. He went so far as to throw out the
conjecture that “comets may become asteroids;” although the converse
proposition that “asteroids may become comets,” of which something has
been heard lately, would scarcely have been entertained by him.

Enough has been said to show how greatly knowledge of the solar system
in all its parts was furthered by Herschel’s observational resources,
fertility of invention, and indomitable energy. He was, so to speak,
ubiquitous. He had taken all the heavens for his province. Nothing that
they included, from the faintest nebula to the sun, and from the sun to
a telescopic shooting-star, evaded his consideration. A whole cycle of
discoveries and successful investigations began and ended with him.

His fame as an astronomer has cast into the shade his merits as
a physicist. He made pioneering experiments on the infra-red
heat-rays,[D] and anticipated, by an admirable intuition, the fact
ascertained with the aid of Professor Langley’s “bolometer,” that
the invisible surpass in extent the visible portions of the solar
spectrum.[E] A search for darkening glasses suitable to solar
observations, led him to the inquiry. Finding that some coloured media
transmitted much heat and little light, while others stopped heat and
let through most of the light, he surmised that a different heating
power might belong to each spectral tint. His own maxim that “it is
sometimes of great use in natural philosophy to doubt of things that
are commonly taken for granted,” here came in appropriately. With a
free mind he set about determining the luminous and thermal powers of
successive spectral regions. They seemed to vary quite disconnectedly.
A thermometer exposed to red rays during a given interval, rose three
and a half times as much as when exposed to violet rays; and he showed
further, by tracing the heat- and light-curves of the prismatic
spectrum, that its heat-maximum lay out of reach of the eye in the
infra-red, while luminous intensity culminated in the yellow. He even
threw out the sagacious conjecture that “the chemical properties of
the prismatic colours” might be “as different as those which relate
to light and heat;” adding that “we cannot too minutely enter into
an analysis of light, which is the most subtle of all the active
principles that are concerned in the operations of nature.”

    [D] Phil. Trans. 1800, p. 255.

    [E] _Ibid._, p. 291.

The ardour with which he pursued the inquiry betrays itself in the
rapid succession of four masterly essays communicated to the Royal
Society in 1800. They contained the first exposition worth mentioning
of the properties of radiant heat. They gave the details of experiments
demonstrating its obedience to the same laws of reflection, refraction,
and dispersion as light; and showing the varieties in the absorptive
action upon it of different substances. In the third memoir of the
series, Professor Holden finds himself at a loss “which to admire
most--the marvellous skill evinced in acquiring such accurate data
with such inadequate means, and in varying and testing such a number
of questions as were suggested in the course of the investigation--or
the intellectual power shown in marshalling and reducing to a system
such intricate, and apparently self-contradictory phenomena.” There
is, indeed, scarcely one of Herschel’s researches in which his
initiative vigour and insight are more brilliantly displayed than in
this _parergon_--this task executed, as it were, out of hours. It is
only a pity that he felt compelled, by the incompatibility of their
distribution in the spectrum, to abandon his original opinion in favour
of the essential identity of light and radiant heat. The erroneous
impression left on the public mind by his recantation has hardly yet
been altogether effaced.




CHAPTER V.

THE INFLUENCE OF HERSCHEL’S CAREER ON MODERN ASTRONOMY.


The powers of the telescope were so unexpectedly increased, that they
may almost be said to have been discovered by William Herschel. No
one before him had considered the advantages of large apertures. No
one had seemed to remember that the primary function of an instrument
designed to aid vision is to collect light. The elementary principle
of space-penetration had not been adverted to. It devolved upon
him to point out that the distances of similar objects are exactly
proportional to the size of the telescopes barely sufficing to show
them. The reason is obvious. Compare, for instance, a one-inch
telescope with the naked eye. The telescope brings to a focus
twenty-five times as much light as can enter the pupil, taken at
one-fifth of an inch in diameter; therefore it will render visible
a star twenty-five times fainter than the smallest seen without its
help; or--what comes to the same thing--an intrinsically equal star
at a five-fold distance. A one-inch glass hence actually quintuples
the diameter of the visible universe, and gives access to seventy-five
times the volume of space ranged through by the unassisted eye.

This simple law Herschel made the foundation-stone of his sidereal
edifice. He was the first to notice it, because he was the first
practically to concern himself with the star-depths. The possibility
of gauging the heavens rose with him above the horizon of science.
Because untiring in exploration, he was insatiable of light; and being
insatiable of light, he built great telescopes.

His example was inevitably imitated and surpassed. Not through a vulgar
ambition to “beat the record,” but because a realm had been thrown open
which astronomers could not but desire to visit and search through for
themselves. Lord Rosse’s six-foot reflector was the immediate successor
of Herschel’s four-foot; Mr. Lassell’s beautiful specula followed; and
the series of large _metallic_ reflectors virtually closed with that of
four-feet aperture erected at Melbourne in 1870. The reflecting surface
in modern instruments is furnished by a thin film of silver deposited
on glass. It has the advantage of returning about half as much again of
the incident light as the old specula, so that equal power is obtained
with less size. Dr. Common’s five-foot is the grand exemplar in this
kind; and it is fully equivalent to the Parsonstown six-foot.

The improvement of refractors proceeded more slowly. Difficulties
in the manufacture of glass stood in the way, and difficulties in
the correction of colour. The splendid success, however, of the Lick
thirty-six inch, and the fine promise of the Yerkes forty-inch, have
turned the strongest current of hope for the future in the direction of
this class of instrument. But all modern efforts to widen telescopic
capacity primarily derive their impulse from Herschel’s passionate
desire to see further, and to see better, than his predecessors.

His observations demonstrate the rare excellence of his instruments.
Experiments made on the asteroid Juno, in 1805, for the purpose
of establishing a valid distinction between real and fictitious
star-discs, prove, in Professor Holden’s opinion, the reflector
employed to have been of almost ideal perfection; and his following of
Saturn’s inner satellites right up to the limb, with the twenty-foot
and the forty-foot, was a _tour de force_ in vision scarcely, if ever,
surpassed.

In the ordinary telescopes of those days really good definition was
unknown; they showed the stars with rays or tails, distorted into
triangles, or bulged into “cocked hats;” clean-cut, circular images
were out of the question. Sitting next Herschel one day at dinner,
Henry Cavendish, the great chemist, a remarkably taciturn man, broke
silence with the abrupt question--“Is it true, Dr. Herschel, that you
see the stars round?” “Round as a button,” replied the Doctor; and no
more was said until Cavendish, near the close of the repast, repeated
interrogatively, “Round as a button?” “Round as a button,” Herschel
briskly reiterated, and the conversation closed.

It seems probable that Herschel’s _caput artis_ lost some of its
fine qualities with time. Great specula are peculiarly liable to
deterioration. Their figure tends to become impaired by the stress of
their own weight; their lustre is necessarily more or less evanescent.
Re-polishing, however, is a sort of re-making; and the last felicitous
touches, upon which everything depends, can never be reckoned upon with
certainty. Hence, the original faultlessness of the great mirror was,
perhaps, never subsequently reproduced.

“Such telescopes as Herschel worked with,” Dr. Kitchiner wrote in
1815, “could only be made by the man who used them, and only be used
by the man who made them.” The saying is strictly true. His skill
in one branch promoted his success in the other. He was as much at
home with his telescopes as the Bedouin are with their horses. Their
peculiarities made part of his most intimate experience. From the
graduated varieties of his specula he picked out the one best suited
to the purpose in hand. It was his principle never to employ a larger
instrument than was necessary, agility of movement being taken into
account no less than capacity for collecting light. The time-element,
indeed, always entered into his calculations; he worked like a man who
has few to-morrows.

His sense of sight was exceedingly refined, and he took care to keep it
so. In order to secure complete “tranquility of the retina,” he used to
remain twenty minutes in the dark before attempting to observe faint
objects; and his eye became so sensitive after some hours spent in
“sweeping,” that the approach of a third-magnitude star obliged him to
withdraw it from the telescope. A black hood thrown over his head while
observing served to heighten this delicacy of vision. He despised no
precaution. Details are “of consequence,” he wrote to Alexander Aubert,
an amateur astronomer, “when we come to refinements, and want to _screw
an instrument up to the utmost pitch_.”

This was said in reference to his application of what seemed
extravagantly high magnifying powers. He laid great stress upon it in
the earlier part of his career. The method, he said, was “an untrodden
path,” in which “a variety of new phenomena may be expected.” With
his seven-foot Newtonian he used magnifications up to nearly 6,000,
proceeding, however, “all along experimentally”--a plan far too much
neglected in “the art of seeing.” “We are told,” he proceeded, “that
we gain nothing by magnifying _too much_. I grant it, but shall never
believe I magnify too much till by experience I find that I can see
better with a lower power.” The innovation was received with a mixture
of wonder, incredulity, and admiration.

Herschel showed his customary judgment in this branch of astronomical
practice. He established the distinctions still maintained, and
laid down the lines still followed. It is true he went far beyond
the point where modern observers find it advisable to stop. The
highest power brought into use with the Lick refractor is 2,600; and
Herschel’s instruments bore 5,800 (nominally 6,500) without injury to
definition. But only at exceptional moments. His habitual sweeping
power was 460; he “screwed-up” higher only for particular purposes,
and under favourable conditions. Although his strong eye-pieces seem,
for intelligible reasons, to have been laid aside on the adoption of
the “front-view” form of construction, they had served him well in
the division of close pairs, as well as for bringing faint stars into
view--an effect correctly explained by him as due to the augmented
darkness, under high powers, of the sky-ground. But the most important
result of their employment was the discovery that the stars have
no sensible dimensions. This became evident through the failure of
attempts to magnify them; the higher the power applied, the smaller and
more intense they appeared. Herschel accordingly pronounced stellar
telescopic discs “spurious,” but made no attempt to explain their
origin through diffraction.

He never possessed an instrument mounted equatoreally--that is, so as
automatically to follow the stars. In its absence, his work, had it not
been accomplished, would have seemed to modern ideas impossible. No
clockwork movement kept the objects he was observing in the field of
view. His hands were continually engaged in supplying the deficiency.
How, under these circumstances, he contrived to measure hundreds of
double stars, and secure the places of thousands of nebulæ, would be
incomprehensible but for the quasi-omnipotence of enthusiasm.

The angle made with the meridian by the line joining two stars (their
“position angle”) was never thought of as a quantity useful to be
ascertained until Herschel, about 1779, invented his “revolving-wire
micrometer.” This differed in no important respect from the modern
“filar micrometer;” only spider-lines have been substituted for the
original silk fibres. For measuring the distances of the wider classes
of double stars, he devised in 1782 a “lamp-micrometer;” while those
of the closest pairs were estimated in terms of the discs of the
components. In compiling his second catalogue, however, he used the
thread-micrometer for both purposes. It is true that “even in his
matchless hands”--in Dr. Gill’s phrase--the results obtained were
“crude;” but the fact remains that the whole system of micrometrical
measurement came into existence through Herschel’s double-star
determinations.

Their consequences have developed enormously within the last few
years. Mr. Burnham’s discoveries of excessively close pairs have been
so numerous as to leave no reasonable doubt that their indefinite
multiplication is only a question of telescopic possibility. Then
in 1889, another power came into play; the spectroscope took up the
work of resolving stars. Or rather, the spectroscope in alliance
with the photographic camera; for the spectral changes indicating
the direction and velocity of motion in the line of sight can be
systematically studied, as a rule, only when registered on sensitive
plates. The upshot has been to bring within the cognisance of science
the marvellous systems known as “spectroscopic binaries.” They are of
great variety. Some consist of a bright, others of a bright and dark,
pair. Those that revolve in a plane nearly coinciding with our line
of vision undergo mutual occultations. A further detachment seem to
escape eclipse, yet vary in light for some unexplained reason, while
they revolve. Others, like Spica Virginis, revolve without varying.
Their orbital periods are counted by hours or days. The study of the
disturbances of these remarkable combinations promises to open a new
era in astronomical theory. For they are most likely all multiple.
Irregularities indicating the presence of attractive, although obscure
bodies, have, in several cases, been already noticed.

The revolutions of spectroscopic binary stars can be studied to the
greatest advantage when they involve light-change; and photometric
methods have accordingly begun to play an important part in the
sidereal department of gravitational science. And here again we meet
with Herschel’s initiative. His method of sequences has been already
explained; and he made the first attempt to lay down a definite scale
of star-magnitudes. He failed, and it was hardly desirable that he
should succeed. On his scale, the ratio of change from one grade to the
next constantly diminished. In the modern system it remains always the
same. A star of the second magnitude is by definition two and a-half
(2·512) times less bright than one of the first; a star of the third
magnitude is two and a-half times less bright than one of the second,
the series descending without modification until beyond telescopic
reach. This uniformity in the _proportionate_ value of a magnitude
is indispensable for securing a practicable standard of measurement.
Herschel, however, took the great step of introducing a principle of
order.

His estimates of stellar lustre were purely visual. And although
various instruments, devised for the purpose, have since proved
eminently useful, the ultimate appeal in all is to the eye. But there
are many signs that, in the photometry of the future, not the eye but
the camera will be consulted. Their appraisements differ markedly.
Herschel’s incidental remark on the disturbance of light-valuation
by colour touches a point of fundamental importance in photographic
photometry. The chemical method gives to white stars a great advantage
over yellow and red ones. They come out proportionately much brighter
on the sensitive plate than they appear to the eye. And to these
varieties of hue correspond spectral class-distinctions, the spectrum
of an object being nothing but its colour written at full length. This
systematic discrepancy between visual and photographic impressions of
brightness, while introducing unwelcome complications in measures of
magnitude, may serve to bring out important truths. The inference, for
example, has been founded upon it that the Milky Way is composed almost
exclusively of white, or “Sirian” stars; and there can be no question
but that the arrangement of stars in space has some respect to their
spectral types.

Herschel’s plan of inquiry into the laws of stellar distribution by
“photometric enumeration,” or gauging by magnitudes, was a bequest
to posterity which has been turned to account with very little
acknowledgment of its source. Argelander’s review of the northern
heavens (lately completed photographically by Dr. Gill to the southern
pole) afforded, from 1862, materials for its application on a large
scale; but the magnitudes assigned to his 324,000 stars do not possess
the regularity needed to make deductions based on them perfectly
trustworthy. Otherwise the distance from the earth of the actual
aggregations in the Milky Way could have been ascertained in a rough
way from the numerical representation of the various photometric
classes. As it is, the presumption is strong that the galactic clouds
are wholly independent of stars brighter than the ninth magnitude--that
they only begin to gather at a depth in space whence light takes _at
least_ a thousand years to travel to our eyes. Confirmatory evidence,
published in 1894, has been supplied by M. Easton’s research, based on
the same principle, into the detailed relations of stars of various
magnitudes to Milky Way structure. They are exhibited only by those of
the ninth magnitude, or fainter; for with them sets in a significant
crowding upon its condensed parts, attended by a scarcity over its
comparative vacuities. Counts by magnitudes have, besides, made it
clear that the stars, in portions of the sky removed from the Milky
Way, thin out notably before the eleventh magnitude is reached; so
that, outside the galactic zone, the stellar system is easily fathomed.

Also on the strength of photometric enumerations, Dr. Gould, of Boston,
came to the conclusion, in 1879, that there is an extra thronging of
stars about our sun, which forms one of a special group consisting
of some four or five hundred members. The publication, in 1890, of
the “Draper Catalogue,” of 10,530 photographed stellar spectra, has
thrown fresh light on this interesting subject. Mr. Monck, of Dublin,
gave reasons for holding stars physically like the sun to be generally
nearer to us than stars of the Sirian class; and Professor Kapteyn, of
Gröningen, as the result of a singularly able investigation, concluded
with much probability that the sun belongs to a strongly condensed
group of mostly “solar” stars, nearly concentric with the galaxy. It
might, in fact, be said that we live in a globular cluster, since our
native star-collection should appear from a very great distance under
that distinctive form.

This modern quasi-discovery was anticipated by Herschel. He was
avowedly indebted, it is true, to Michell’s “admirable idea” of the
stars being divided into separate groups; but Michell did not trouble
himself about the means of its possible verification, and Herschel did.
He always looked round to see if there were not some touchstone of fact
within reach.

His discussion of the solar cluster, though brief and incidental, is
not without present interest. He found the federative arrangement of
the stars to be “every day more confirmed by observation.” The “flying
synods of worlds” formed by them must gravitate one towards another as
if concentrated at their several centres of gravity. Accordingly, “a
star, or sun, such as ours, may have a proper motion within its own
system of stars, while the whole may have another proper motion totally
different in quantity and direction.” We may thus, he continued,
“arrive in process of time, at a knowledge of all the real, complicated
motions of the planet we inhabit; of the solar system to which it
belongs; and even of the sidereal system of which the sun may possibly
be a member.” He proceeded to explain how stars, making part of the
solar cluster, might be discriminated from those exterior to it; the
former showing the perspective influence only of the sun’s translation
among themselves, while the latter would be affected besides by a
“still remoter parallax”--a secular drift, compounded of the proper
motion of the sun within its cluster, and of its cluster relatively to
other clusters.

The possibility of applying Herschel’s test is now fully recognised.
Each fresh determination of the solar apex is scrutinised for symptoms
of the higher “systematical parallax;” although as yet with dubious
or negative results. Associated stellar groups are, nevertheless, met
with in various parts of the sky. Herschel not only anticipated their
existence, but suggested “a concurrence of proper motions” as the
fittest means for identifying them.

His anticipation has been realised by Mr. Proctor’s detection of
“star-drift.” Several stars in the Plough thus form a squadron sailing
the same course; and similar combinations, on an apparently smaller
scale, have been pieced together in various constellations. But the
principle of their connection has yet to be discovered. They are
evidently not self-centred systems; hence their companionship, however
prolonged, must finally terminate. The only pronounced cluster with a
common proper motion is the Pleiades; and its drift seems to be merely
of a perspective nature--a reflection of the sun’s advance.

Bessel said of Herschel that “he aimed at acquiring knowledge, not of
the motions, but of the constitution of the heavenly bodies, and of
the structure of the sidereal edifice.” This, however, is a defective
appreciation. He made, indeed, no meridian observations, and computed
no planetary or cometary perturbations; yet if there ever was an
astronomer who instinctively “looked before and after,” it was he.
Could he have attained to a complete knowledge of the architecture
of the heavens, as they stood at a given moment, it would not have
satisfied him. To interpret the past and future by the present was his
constant aim; from his “retired situation” on the earth, he watched
with awe the grand procession of the sum of things defile through
endless ages. He could not observe what was without at the same time
seeking to divine what had been, and to forecast what was to come.

His nebular theory is now accepted almost as a matter of course. The
spectroscope has lent it powerful support by proving the _de facto_
existence of the “lucid medium,” postulated by him as a logical
necessity. This was done August 1st, 1864, when Dr. Huggins derived
from a planetary nebula in Draco a spectrum characteristic of a gaseous
body, because consisting of bright lines. Their wave-lengths, which
turned out to be identical for all objects of the kind, with one or
two possible exceptions, indicated a composition out of hydrogen
mixed with certain unfamiliar aeriform substances. Herschel’s visual
discrimination of gaseous nebulæ was highly felicitous. Modern science
agrees with him in pronouncing the Orion nebula, as well as others
of the irregular class, planetaries, diffused nebulosities, and the
“atmospheres” of “cloudy stars,” to be masses of “shining fluid.” As
for his “ambiguous objects,” they remain ambiguous still. “Clusters
in disguise” through enormous distance, give apparently the same
quality of light with irresolvable nebulæ. His inference that stars
and nebulæ form mixed systems has, moreover, been amply confirmed. No
one now denies their significant affinity, and very few their genetic
relationship.

Herschel gave a list in 1811 of fifty-two dim, indefinite nebulosities,
covering in the aggregate 152 square degrees. “But this,” he added,
“gives us by no means the real limits” of the luminous appearance;
“while the depth corresponding to its superficial extent may be far
beyond the reach of our telescopes;” so “that the abundance of nebulous
matter diffused through such an expansion of the heavens must exceed
all imagination.”

“The prophetic spirit of these remarks,” Professor Barnard comments,
“is being every day made more evident through the revelations of
photography.” He is himself one of the very few who have telescopically
verified any part of these suggestive observations.

“I am familiar,” he wrote in _Knowledge_, January, 1892, “with a number
of regions in the heavens where vast diffusions of nebulous matter are
situated. One of these, in a singularly blank region, lies some five
or six degrees north-west of Antares, and covers many square degrees.
Another lies north of the Pleiades, between the cluster and the Milky
Way; a portion of this has recently been successfully photographed
by Dr. Archenhold. There is a large nebulous spot in that region,
easily visible to the naked eye, which I have seen for many years. When
sweeping there with a low power, the whole region between the Pleiades
and the Milky Way is perceived to be nebulous. These great areas of
nebulosity make their presence known by a singular dulling of the
ordinarily black sky, as if a thin veil of dust intervened.” They “are
specially suitable for the photographic plate, and it is only by such
means that they can be at all satisfactorily located.”

Some of Herschel’s milky tracts have been thus pictured; notably one
in the Swan, shown on Dr. Max Wolf’s plates to involve the bright star
Gamma Cygni; and another immense formation extending over sixty square
degrees about the belt and sword of Orion, and joining on, Herschel was
“pretty sure,” to the great nebula. This, never unmistakably _seen_
except by him, portrayed itself emphatically in 1886 in Professor E.
C. Pickering’s photographs. Herschel’s persuasion of the subordinate
character of the original “Fish-mouth nebula” was well-grounded.
On plates exposed by Professors W. H. Pickering and Barnard, it is
disclosed as the mere nucleus of a tremendous spiral, sweeping round
from Bellatrix to Rigel.

Diffused nebulosities appear in photographs as far from homogeneous.
They are not simple volumes of gas indefinitely expanding in all
directions, after the manner of simple aeriform fluids. They possess,
on the contrary, characteristic shapes. Structureless nebulæ, like
structureless protoplasm, seem to be non-existent. In all, an
organising principle is at work.

Minute telescopic stars showed to Herschel as prevalently red, owing,
he conjectured, to the enfeeblement of their blue rays during an
uncommonly long journey through space “not quite destitute of some very
subtle medium.” The argument is a remarkable one. It would be valid if
the ethereal vehicle of light exercised absorption after the manner of
ordinary attenuated substances. There is, however, reason to suppose
that the symptomatic redness was only a subjective impression, not an
objective fact. His colour-sense was not quite normal. The lower, to
his perception, somewhat overbalanced the higher end of the spectrum,
and his mirrors added to the inequality by reflecting a diminished
proportion of blue light. Thus he recorded many stars as tinged with
red which are now colourless, yet lie under no suspicion of change.

Herschel was, in the highest and widest sense, the founder of sidereal
astronomy. He organised the science and set it going; he laid down
the principles of its future action; he accumulated materials for its
generalisations, and gave examples of how best to employ them. His work
was at once so stimulating and so practical that its abandonment might
be called impossible. Others were sure to resume where he had left
off. His son was his first and fittest successor; he was the only one
who undertook in its entirety the inherited task. Yet there are to be
found in every quarter of the world men imbued with William Herschel’s
sublime ambitions. Success swells the ranks of an invading army; and
the march of astronomy has, within the last decade, assumed a triumphal
character. The victory can never be completely won; the march can never
reach its final goal; but spoils are meanwhile gathered up by the
wayside which eager recruits are crowding in to share. The heavens
are, year by year, giving up secrets long and patiently watched for,
while holding in reserve many others still more mysterious. There is no
fear of interest being exhausted by disclosure.

Herschel’s dim intuition that something might be learned about the
physical nature of the stars from the diverse quality of their light,
was verified after sixty-five years, by the early researches of
Secchi, Huggins, and Miller; but he could not suspect that, through
the chemical properties, which he guessed to belong in varying degrees
to the different sections of their spectra, pictures of the heavenly
bodies would be obtained more perfect than the telescopic views he
rapturously gazed at. Still less could he have imagined that, owing
to its faculty of accumulating impressions too weak to affect the
eye separately, the chemical would, in great measure, supersede the
telescopic method in carrying out the designs he had most at heart.

Those designs have now grown to be of international importance. At
eighteen northern and southern observatories a photographic review
of the heavens is in progress. The combined results will be the
registration, in place and magnitude, of fifteen to twenty millions
of stars. The gauging of the skies will then be complete down to the
fourteenth magnitude; and the “construction of the heavens” can be
studied with materials of the best quality, and almost indefinite
in quantity. By simply “counting the gauges” on Herschel’s early
plan, much may be learnt; the amount of stellar condensation
towards the plane of the Milky Way, for instance, and the extent
of stellar denudation near its poles. A marked contrast between
the measures of distribution in these opposite directions will most
likely be brought into view. The application of his later method of
enumeration by magnitudes ought to prove even more instructive, but
may be very difficult. The obstacles, it is to be hoped, will not be
insurmountable; yet they look just now formidable enough.

The grand problem with which Herschel grappled all his life involves
more complicated relations than he was aware of. It might be compared
to a fortress, the citadel of which can only be approached after
innumerable outworks have been stormed. That one man, urged on by
the exalted curiosity inspired by the contemplation of the heavens,
attempted to carry it by a _coup de main_, and, having made no
inconsiderable breach in its fortifications, withdrew from the
assault, his “banner torn, but flying,” must always be remembered with
amazement.

[Illustration: CAROLINE LUCRETIA HERSCHEL.

(_From a portrait taken by Tielemann in 1829._)]




CHAPTER VI.

CAROLINE HERSCHEL.


Caroline Lucretia Herschel was born at Hanover, March 16th, 1750, and
was thus more than eleven years younger than the brother with whose
name hers is inseparably associated. She remembered the panic caused
by the earthquake of 1755, and her experience barely fell short of the
political earthquake of 1848; but the fundamental impressions of her
long life were connected with “minding the heavens.”

She was of little account in her family, except as a menial. Her
father, indeed, a man of high character and cultivated mind, thought
much of her future, and wished to improve her prospects by giving her
some accomplishments. So he taught her to play the violin well enough
to take part in concerted music. But her instruction was practicable
only when her mother was out of the way, or in a particularly good
humour. Essentially a “Hausfrau,” Anna Ilse had no sympathy with
aspirations. She was hard-working and well-meaning, but narrow and
inflexible, and she kept her second daughter strictly to household
drudgery. Her literary education, accordingly, got no farther than
reading and writing; even the third “R” was denied to her. But she was
carefully trained in plain sewing and knitting, and supplied her four
brothers with stockings from so early an age that the first specimen of
her workmanship touched the ground while she stood upright finishing
the toe! Few signs of tenderness were accorded to her. Her eldest
brother, Jacob, a brilliant musician, and somewhat high-and-mighty
in his ways, did not spare cuffs when she waited awkwardly at table;
and her sister, Mrs. Griesbach, evidently took slight notice of her.
William, however, showed her invariable affection; and him and her
father she silently adored. In 1756, when they both returned from
England with the Hanoverian Guard, she recalled how, on the day of
their arrival,

“My mother being very busy preparing dinner, had suffered me to go
all alone to the parade to meet my father, but I could not find him
anywhere, nor anybody whom I knew; so at last, when nearly frozen to
death, I came home and found them all at table. My dear brother William
threw down his knife and fork, and ran to welcome, and crouched down to
me, which made me forget all my grievances. The rest were so happy at
seeing one another again that my absence had never been perceived.”

How well one can realise the disconsolate little expedition, the
woe-begone entry of the six-year-old maiden, her heart-chill on finding
herself forgotten, and the revulsion of joy at her soldier-brother’s
cordial greeting!

Isaac Herschel died March 22nd, 1767. He had never recovered the
campaign of Dettingen, yet struggled, in spite of growing infirmities,
to earn a livelihood by giving lessons and copying music. His daughter
was thrown by his loss into a “state of stupefaction,” from which she
roused herself, after some weeks, to consider the gloomy outlook of
her destiny. She was seventeen, and was qualified, as she reflected
with anguish, only to be a housemaid. She was plain in face and
small in stature, and her father had often warned her that if she
ever married it would be comparatively late in life, when her fine
character had unfolded its attractions. Still, she did not lose hope
of making her way single-handed. Although over-burthened with servile
labours, she contrived, unknown to her mother, to get some teaching in
fancy-work from a consumptive girl whose cough from across the street
gave the signal for a daybreak rendezvous; trusting that, with this
acquirement, and “a little notion of music, she might obtain a place
as governess in some family where the want of a knowledge of French
would be no objection.” There was “no kind of ornamental needlework,
knotting, plaiting hair, stringing beads and bugles, of which she did
not make samples by way of mastering the art.” She was then permitted
to take some lessons in dressmaking and millinery. But the current of
her thoughts was completely changed by an invitation from her brother
William to join him at Bath. She was, if possible, to be made into
a concert-singer. Yet her voice had never been tried, and its very
existence was problematical. It may, then, be suspected that William’s
primary motive was to come to the rescue of his poor little Cinderella
sister.

Months passed in “harassing uncertainty” as to whether she was to go or
stay; months, too, during which her own mind was divided between the
longing to follow her rising star, and a certain compunctious clinging
to her duties at home. Time, however, did not pass in idleness.
Taking no notice of the superior Jacob’s ridicule of her visionary
transformation into an artist, she quietly set about practising, with a
gag between her teeth, the solo parts of violin concertos, “shake and
all,” so that, as she says, “I had gained a tolerable execution before
I knew how to sing.” She occupied herself besides in making a store of
prospective clothing for relatives, who, she could not but fear, would
miss her services. For her withdrawal her mother, however, received
from William money-compensation, which enabled her to keep a servant
in lieu of her daughter. The parting, when he came to fetch her, in
August, 1772, was none the less a sorrowful one; but Caroline had much
to distract her mind from dwelling on those she had left behind. She
had, besides, much discomfort to endure. Six days and nights in an
open stage-carriage were followed by a tempestuous passage; the packet
in which they embarked at Helvoetsluys reached Yarmouth dismasted and
half-wrecked; and they were finally, not duly landed, but “thrown like
balls by two sailors,” on the English coast. After a brief glimpse of
London, they started, August 28th, in the night coach for Bath, where
Caroline arrived “almost annihilated” by fatigue and want of sleep.

Her training for an unfamiliar life began without delay. She had to
learn English, arithmetic, and enough of account-keeping to qualify
her for conducting the household affairs; a routine of singing-lessons
and practising was entered upon; and she was sent out alone to market,
Alexander Herschel lurking behind to see that she came safely out of
the _mêlée_ of buyers and sellers, whence she brought home “whatever
in her fright she could pick up.” She suffered many things, too, from
her brother’s servant, “a hot-headed old Welshwoman,” whose _régime_
was one of rack and ruin to domestic utensils; while _heimweh_ made
formidable onslaughts on her naturally serene spirits.

A visit to London, as the guest of Mrs. Colebrook, one of her
brother’s pupils, gave her some experience of town gaieties. But the
expenses of dress and chairmen shocked her frugal ideas; and she
thought the young ladies, whose companionship was offered to her, “very
little better than idiots.” As a vocalist, Miss Herschel came easily
to the front. After a few months of study, her voice was in demand at
evening parties; when her foreign accentuation had been corrected,
she took the first soprano parts in “The Messiah,” “Samson,” “Judas
Maccabæus,” and other oratorios; and sang as prima donna at the winter
concerts both at Bath and Bristol. In accordance with her resolution
to appear only where her brother conducted, she declined an engagement
for a musical festival at Birmingham. A year’s training in deportment
was a preliminary to her _début_; a celebrated dancing mistress
being engaged--to use Caroline’s own phrase--“in drilling me for a
gentlewoman. Heaven knows how she succeeded!” A gift of ten guineas
from William provided her with a dress which made her, she was told,
“an ornament to the stage;” and she was complimented by the Marchioness
of Lothian on “pronouncing her words like an Englishwoman.” Her success
was decided, and promised to be enduring enough to satisfy her modest
ambition of supporting herself independently.

It was, however, balked by an extraordinary turn of affairs; a turn
at first not at all to her liking. After the lapse of half-a-century
she still set it down as the grievance of her life that “I have been
throughout annoyed and hindered in my endeavours at perfecting myself
in any branch of knowledge by which I could hope to gain a creditable
livelihood.”

William Herschel, when Caroline joined him at Bath, was just feeling
his way towards telescope-making. The fancy did not please her. The
beginnings of great things are usually a disturbance and an anxiety.
They imply a draft upon the future which may never be honoured, and
they often play sad havoc with the present. And Miss Herschel was
business-like and matter-of-fact. But her devotion triumphed over her
common-sense. Keeping her misgivings to herself, she met unlooked-for
demands with the utmost zeal, intelligence, and discretion. She was
always at hand when wanted, yet never in the way. Through her care,
some degree of domestic comfort was maintained amid the unwonted
confusion of optical manufacture. During the tedious process of
mirror-polishing, she sustained her brother physically and mentally,
putting food into his mouth, and reading aloud “Don Quixote,” and the
“Arabian Nights.” She was ready with direct aid, too, and “became in
time as useful a member of the workshop as a boy might be to his master
in the first year of his apprenticeship.” “Alex,” she continued, “was
always very alert, assisting when anything new was going forward;
but he wanted perseverance, and never liked to confine himself at
home for many hours together. And so it happened that my brother
William was obliged to make trial of my abilities in copying for him
catalogues, tables, and sometimes whole papers which were lent him
for his perusal.” Musical business, meantime, received due attention.
Steady preparation was made for concerts and oratorios; choruses were
instructed, rehearsals attended, parts diligently written out from
scores. But the discovery of Uranus swept away the necessity for these
occupations; and with a final performance in St. Margaret’s Chapel, on
Whit-Sunday, 1782, the musical career of William and Caroline Herschel
came to a close.

Miss Herschel’s “thoughts were anything but cheerful” on the occasion.
She saw the terrestrial ground cut from under her feet, and did not
yet appreciate the celestial situation held in reserve for her. Music,
in her opinion, was her true and only vocation; the contemplation
of herself in the guise of an assistant-astronomer moved her to
cynical self-scorn. As usual, however, her personal wishes were
suppressed. Housewifely cares, too, weighed upon her. The dilapidated
gazebo at Datchet provided no suitable shelter for a well-regulated
establishment. It was roofed more in appearance than in reality; the
plaster fell from the ceilings; the walls dripped with damp; rheumatism
and ague were its rightful inmates. Then the prices of provisions
appalled her, especially in view of the scarcity of five-pound notes
since the opulence of Bath had been exchanged for the penury of a court
precinct.

Yet she set to work with a will to learn all that was needful for her
untried office. Not out of books. “My dear brother William,” she wrote
in 1831, “was my only teacher, and we began generally where we should
have ended; he supposing I knew all that went before.” The lessons were
of the most desultory kind. They consisted of answers to questions put
by her as occasions arose, during breakfast, or at odd moments. The
scraps of information thus snatched were carefully recorded in her
commonplace book, where they constituted a miscellaneous jumble of
elementary formulæ, solutions of problems in trigonometry, rules for
the use of tables of logarithms, for converting sidereal into solar
time, and the like. Nothing was entrusted to a memory compared by
her instructor to “sand, in which everything could be inscribed with
ease, but as easily effaced.” So that even the multiplication table was
carried about in her pocket. She appears never to have spent a single
hour in the systematic study of astronomy. Her method was that in vogue
at Dotheboys Hall, to “go and know it,” by practising, as it were,
blindfold, what she had been taught. Yet a computational error has
never, we believe, been imputed to her; and the volume of her work was
very great.

Its progress was diversified by more exciting pursuits. She began, in
1782, to “sweep for comets,” and discovered with a 27-inch reflector,
in the autumn of 1783, two nebulæ of first-rate importance--one
a companion to the grand object in Andromeda, the other a superb
elliptical formation in Cetus. She was by this time more than
reconciled to her astronomical lot; Von Magellan, indeed, reported in
1785, that brother and sister were equally captivated with the stars.

The original explorations, in which she was beginning to delight, were
interrupted by the commencement of his with the “large twenty-foot.”
Her aid was indispensable, and from December, 1783, she “became
entirely attached to the writing-desk.” She was no mere mechanical
assistant. A wound-up automaton would have ill served William
Herschel’s turn. He wanted “a being to execute his commands with the
quickness of lightning”; and his commands were various. For he was
making, not following precedents, and fresh exigencies continually
arose. Under these novel circumstances, his sister displayed incredible
zeal, promptitude, and versatility. She would throw down her pen to
run to the clock, to fetch and carry instruments, to measure the ground
between the lamp-micrometer and the observer’s eye; discharging these,
and many other successive tasks with a rapidity that kept pace with
his swift proceedings. Fatigue, want of sleep, cold, were disregarded;
and although nature often exacted next day penalties of weariness
and depression for those nights of intense activity, the faithful
amanuensis never complained. “I had the comfort,” she remarked simply,
“to see that my brother was satisfied with my endeavours to assist
him.” The service was not unaccompanied by danger. One night poor
Caroline, running in the dark over ground a foot deep in melting snow,
in order to make some alteration in the movement of the telescope,
fell over a great hook, which entered her leg so deeply that a couple
of ounces of her flesh remained behind when she was lifted off it.
The wound was formidable enough, in Dr. Lind’s opinion, to entitle a
soldier to six weeks’ hospital-nursing, but it was treated cursorily at
Datchet; the patient consoling herself for a few nights’ disablement
with the reflection that her brother, owing to cloudy weather, “was no
loser through the accident.”

Busy days succeeded watchful nights. From the materials collected at
the telescope, she formed properly arranged catalogues, calculating, in
all, the places of 2,500 nebulæ. She brought the whole of Flamsteed’s
_British Catalogue_--then the _vade mecum_ of astronomers--into
zones of one degree wide, for the purpose of William’s methodical
examination; copied out his papers for the Royal Society; kept the
observing-books straight, and documents in order. Then, in the long
summer months, when “there was nothing but grinding and polishing to
be seen,” she took her share of that too, and “was indulged with the
last finishing of a very beautiful mirror for Sir William Watson.”

On August 1st, 1786, her brother’s absence leaving her free to observe
on her own account, she discerned a round, hazy object, suspiciously
resembling a comet. Its motion within the next twenty-four hours
certified it as such, and she immediately announced the apparition to
her learned friends, Dr. Blagden and Mr. Aubert. The latter declared in
reply, “You have immortalised your name,” and saw in imagination “your
wonderfully clever and wonderfully amiable brother shedding,” upon
receipt of the intelligence, “a tear of joy.” This was the first of a
series of eight similar discoveries, in five of which her priority was
unquestioned. They were comprised within eleven years, and were made,
after 1790, with an excellent five-foot reflector mounted on the roof
of the house at Slough. Considering that she swept the heavens only as
an interlude to her regular duties, never for an hour forsaking her
place beside the great telescopes in the garden, her aptitude for that
fascinating pursuit must be rated very high. It was not until 1819 that
Encke identified her seventh comet--detected November 7th, 1795--with
one previously seen by Méchain in January, 1786. None other revolves
so quickly, its returns to perihelion occurring at intervals of three
and a quarter years. It has earned notoriety, besides, by a still
unexplained acceleration of movement.

Caroline Herschel was the first woman to discover a comet; and her
remarkable success in what Miss Burney called “her eccentric vocation,”
procured for her an European reputation. But the homage which she
received did not disturb her sense of subordination. “Giving the sum of
more to that which hath too much,” she instinctively transferred her
meed of praise to her brother. She held her comets, notwithstanding,
very dear. All the documents relating to them were found after her
death neatly assorted in a packet labelled “Bills and Receipts of my
Comets”; and the telescopes with which they had been observed ranked
among the chief treasures of her old age. She presented the smaller one
before her death to her friend Mr. Hausmann; the five-foot to the Royal
Astronomical Society, where it is religiously preserved.

The “celebrated comet-searcher” was described by Miss Burney in 1787
as “very little, very gentle, very modest, and very ingenuous; and her
manners are those of a person unhackneyed and unawed by the world,
yet desirous to meet and return its smiles.” To Dr. Burney, ten years
later, she appeared “all shyness and virgin modesty”; while Mrs.
Papendick mentions her as “by no means prepossessing, but an excellent,
kind-hearted creature.” She was, in 1787, officially appointed her
brother’s assistant, with a salary of fifty pounds a year; “and in
October,” she relates, “I received twelve pounds ten, being the first
quarterly payment of my salary, and the first money I ever in all my
lifetime thought myself to be at liberty to spend to my own liking.”
The arrangement was made in anticipation of her brother’s marriage,
when--to quote her one bitter phrase on the subject--“she had to give
up the place of his housekeeper.” She did not readily accommodate
herself to the change; and a significant gap of ten years in her
journal suggests that she wrote much during that time of struggle
which her calmer judgment counselled her to destroy. Her strong sense
of right and habitual abnegation, however, came to her aid; the family
relations remained harmonious; and she eventually became deeply
attached to her gentle sister-in-law. But from 1788 onwards, she lived
in lodgings, either at Slough or Upton, whence she came regularly to
the observatory to do her daily or nightly work.

Miss Herschel began in 1796, and finished in about twenty months,
an Index to Flamsteed’s observations of the stars in the “British
Catalogue.” A list of “errata” was added, together with a catalogue of
561 omitted stars. The work, one of eminent utility, was published in
1798, at the expense of the Royal Society. In August, 1799, she paid
a visit to the Astronomer Royal, with the object of transcribing into
his copy of Flamsteed’s Observations some memoranda upon them made by
her brother. “But the succession of amusements,” we hear, “left me no
alternative between contenting myself with one or two hours’ sleep per
night during the six days I was at Greenwich, and going home without
having fulfilled my purpose.” Needless to say that she chose the former.

The Royal family paid her many attentions, partly, no doubt, because
of her intimacy with one of the ladies-in-waiting to the Queen.
This was Madame Beckedorff, who although of “gentle” condition, had
attended the same dressmaking class with the bandmaster’s daughter at
Hanover, in 1768. The distant acquaintanceship thus formed developed,
at Windsor, into a firm friendship, transmitted in its full cordiality
to a second generation. An entry in Caroline’s Diary tells of a dinner
at Madame Beckedorff’s, February 23, 1801, when the “whole party
left the dining-room on the Princesses Augusta and Amelia, and the
Duke of Cambridge coming in to see me.” In May, 1813, during a visit
to London, she passed several evenings at Buckingham House, “where I
just arrived,” she says, on May 12, “as the Queen and the Princesses
Elizabeth and Mary, and the Princess Sophia Matilda of Gloucester,
were ready to step into their chairs, going to Carlton House, full
dressed for a fête, and meeting me in the hall, they stopped for near
ten minutes, making each in their turn the kindest inquiries how I
liked London, etc. On entering Mrs. Beckedorff’s room, I found Madame
D’Arblay (Miss Burney), and we spent a very pleasant evening.”

Such Royal condescensions were frequent, and on occasions inconvenient.
The Princesses Sophia and Amelia, in especial, took a strong liking
for Miss Herschel’s conversation, and often required her attendance
for many hours together. She was graciously singled out for notice at
the Frogmore assemblages, and became quite inured to the reception
at Slough of dignitaries and _savants_. Nothing deranged the simple
composure of her deportment. One would give much to know what were her
private impressions about the notabilities who crossed her path; but
her memoranda are, in this respect, perfectly colourless. Names and
dates are jotted down with the same brevity as her entries of “work
done.” Even the personal troubles of years are curtly disposed of. Her
brother Dietrich’s stay in England from 1809 to 1813, left her not a
day’s respite from accumulated trouble and anxiety. Yet it occasioned
only one little outburst, penned long afterwards.

“He came,” she wrote, “ruined in health, spirit, and fortune, and,
according to the old Hanoverian custom, I was the only one from whom
all domestic comforts were expected. I hope I acquitted myself to
everybody’s satisfaction, for I never neglected my eldest brother’s
business” (Jacob Herschel died in 1792), “and the time I bestowed on
Dietrich was taken entirely from my sleep, or what is generally allowed
for meals, which were mostly taken running, or sometimes forgotten
entirely. But why think of it now?”

Her later journal is overshadowed with the fear of coming bereavement.
Recurrences to the state of William’s health become ominously frequent.
“He is not only unwell, but low in spirits,” she notes in February,
1817; and the following account of his departure for Bath, April 2,
1818, betrays her deep trouble:--

“The last moments before he stepped into the carriage were spent in
walking through his library and workrooms, pointing with anxious looks
to every shelf and drawer, desiring me to examine all, and to make
memorandums of them as well as I could. He was hardly able to support
himself, and his spirits were so low, that I found difficulty in
commanding my voice so far as to give him the assurance he should find
on his return that my time had not been misspent.”

“May 1st.--But he returned home much worse than he went, and for
several days hardly noticed my handiworks.”

His last note to her, indited with an uncertain hand on a discoloured
slip of paper, July 4, 1819, she put by with the inscription: “I keep
this as a relic. Every line _now_ traced by the hand of my dear brother
becomes a treasure to me.”

“Lina,” it ran, “there is a great comet. I want you to assist me. Come
to dine and spend the day here. If you can come soon after one o’clock
we shall have time to prepare maps and telescopes. I saw its situation
last night--it has a long tail.”

Through that long tail the earth had, eight days previously--according
to Olbers’s calculations--cut its way; but the proposed observations at
Slough, if made, were never published.

In October, 1821, Caroline Herschel wrote this melancholy “Finis” to
what seemed to herself the only part of her life worth living. “Here
closed my day-book; for one day passed like another, except that I,
from my daily calls, returned to my solitary and cheerless home with
increased anxiety for each following day.”

Eighteen months after her loss of “the dearest and best of brothers,”
she at last gathered fortitude to put on paper her recollections of the
“heartrending occurrences” witnessed by her during the closing months
of her fifty years’ sojourn in England. In every line of what she then
wrote, her absorbed fidelity to him, growing more and more tenacious
as the end drew visibly nigher, comes out with unconscious pathos. The
anguish with which she watched each symptom of decay seared her heart,
but was refused any outward expression. She played out her rôle of
self-suppression until the curtain fell. A last gleam of hope visited
her July 8th, 1822, when she marked down in an almanac the cheering
circumstance that her invalid had “walked with a firmer step than usual
above three or four times the distance from the dwelling-house to the
library, in order to gather and eat raspberries in his garden with me.
But,” she added sadly, “I never saw the like again.”

In the impetuosity of her grief, she made an irreparable mistake. Only
a month earlier she had surrendered to her impecunious brother Dietrich
her little funded property of £500; now, without reflecting on the
consequences, she “gave herself, with all she was worth, to him and his
family.” She was in her seventy-third year; her only remaining business
in life, it seemed to her, was to quit it; the virtual close of her
career had come; the actual close could not long be delayed. So she
retired to her native place to die promptly, if that might be, but, at
any rate, to mark the chasm that separated her from the past. She soon
recognised, however, that she had taken a false step. “Why did I leave
happy England?” was the cry sometimes on her lips, always in her heart,
for a quarter of a century. She was taken aback by her own vitality.
She found out too late that her powers of work, far from being
exhausted, might have been turned to account for her nephew as they had
been for her brother. And it was to him and his mother, after all, that
her strong affections clung. Her relatives in Hanover, although they
treated her with consideration, were hopelessly uncongenial. “From the
moment I set foot on German ground,” she said, “I found I was alone.”
Fifty years is a huge gap in a human life. Miss Herschel had been all
that time progressing from the starting point where they had remained
stationary. Their tastes were then necessarily incongruous with hers;
nor could her interests be transplanted at will from the soil in which
they were rooted. She was unable to perceive that the change was in
herself. The “solitary and useless life” she led resulted, she was
convinced, from her “not finding Hanover, or anyone in it, like what I
left when the best of brothers took me with him to England in August,
1772!”

An exile in her old home, she felt pledged to remain there. She would
not “take back her promise.” For a person of her frugal habits, she was
well off. Her pension of fifty pounds would have supplied her small
wants, and she was reluctantly compelled to accept the annuity of £100,
left to her by her brother. And since she was most generous in the
bestowal of her spare cash, her presence was of some material advantage
to a poor household. It gave them credit, too; and notwithstanding that
they “never could agree” in opinions, she faithfully nursed Dietrich
Herschel until his death in January, 1827.

“I am still unsettled,” she wrote to her nephew, December 26th, 1822,
“and cannot get my books and papers in any order, for it is always noon
before I am well enough to do anything, and then visitors run away with
the rest of the day till the dinner-hour, which is two o’clock. Two or
three evenings in each week are spoiled by company. And at the heavens
there is no getting, for the high roofs of the opposite houses. But
within my room I am determined nothing shall be wanting that can please
my eye. Exactly facing me is a bookcase placed on a bureau, to which I
will have some glass doors made, so that I can see my books. Opposite
this, on a sofa, I am seated, with a sofa-table and my new writing-desk
before me; but what good I shall do there the future must tell.”

Seated at that “new desk,” she completed her most important work. This
was the reduction into a catalogue, and the arrangement into zones, of
all Sir William Herschel’s nebulæ and clusters. Despatched to Sir John
Herschel in April, 1825, it made his review of those objects feasible.
From it, he drew up his “working-list” for each night’s observations;
and from it, in constructing his “General Catalogue” of 1864, he
took the places of such nebulæ as he had not been able to examine
personally. In the course of the needful comparisons, “I learned,” he
said, “fully to appreciate the skill, diligence, and accuracy which
that indefatigable lady brought to bear on a task which only the most
boundless devotion could have induced her to undertake, and enabled
her to accomplish.” For its execution, the Gold Medal of the Royal
Astronomical Society was awarded to her in 1828--an honour by which
she was “more shocked than gratified.” Her “Zone-Catalogue” was styled
by Sir David Brewster “an extraordinary monument of the unextinguished
ardour of a lady of seventy-five in the cause of abstract science.”

In 1835, she was created an honorary member of the Royal Astronomical
Society, Mrs. Somerville being associated with her in a distinction
never before or since conferred upon a woman. Three years later, she
was surprised by the news that the Royal Irish Academy had similarly
enrolled her. “I cannot help,” she wrote, “crying out aloud to myself,
every now and then, What is that for?” The arrival, on another
occasion, of presentation-copies of Mrs. Somerville’s “Connexion of the
Physical Sciences,” and of Baily’s “Account of Flamsteed,” agitated her
painfully. “Coming to _me_ with such things,” she exclaimed, “an old,
poor, sick creature in her dotage.” “I think it is almost mocking me,”
she added in 1840, “to look upon me as a Member of an Academy; I that
have lived these eighteen years without finding as much as a single
comet.”

Her local celebrity, nevertheless, diverted her. It struck her as a
capital joke that she was “stared at for a learned lady.” Down to 1840
she regularly attended plays and concerts, and rarely left the theatre
without a “_Wie geht’s?_” from His Majesty. And to find herself--“a
_little_ old woman”--conspicuous in the crowd, produced a sense of
exhilaration. Her presence or absence was a matter of public concern,
and she very seldom appeared otherwise than alert and cheerful. When
close upon eighty her “nimbleness in walking,” she remarked, “has
hitherto gained me the admiration of all who know me; but the good
folks are not aware of the arts I make use of, which consist in never
leaving my room in the daytime except I am able to trip it along as
if nothing were the matter.” Music gave her unfailing pleasure. She
heard Catalani in 1828; shared in the Paganini _furore_ of 1831, and
conversed with him through an interpreter. With Ole Bull she was
“somewhat disappointed,” finding his performance “more like conjuration
than playing on a violin.”

But her “painful solitude” was most of all cheered by the visits and
communications of eminent men. No one of distinction in science came
to Hanover without calling upon her. Humboldt, Gauss, Mädler, Encke,
Schumacher, paid her their respects, personally or by letter, if not in
both ways. “Next to listening to the conversation of learned men,” she
told the younger Lady Herschel, “I like to hear about them; but I find
myself, unfortunately, among beings who like nothing but smoking, big
talk on politics, wars, and such-like things.” Her situation remained,
to the end, displeasing to her. She made the best of it; but the best
was, to her thinking, bad. Having wilfully flung herself out of the
current of life, she was nevertheless surprised at being stranded.
She recurred, with inextinguishable pain, to the crippling effects of
circumstances and old age.

“I lead a very idle life,” she wrote in 1826. “My sole employment
consists in keeping myself in good humour, and not being disagreeable
to others.” And in 1839: “I get up as usual, every day, change my
clothing, eat, drink, and go to sleep again on the sofa, except I am
roused by visitors; then I talk till I can talk no more--nineteen to
the dozen!” While at nights “the few, few stars I can get at out of my
window only cause me vexation, for to look for the small ones on the
globe my eyes will not serve me any longer.”

She followed, however, with intense delight the progress of her
nephew’s career, in which she beheld the continuation of his father’s.
The intelligence of his having opened a nebular campaign in 1825, was
like the sound of the trumpet to a disabled war-horse. Nothing but
the decline of her powers, she assured him, would have prevented her
“coming by the first steamboat to offer you the same assistance as, by
your father’s instructions, I was enabled to afford him.” And again,
in 1831: “You have made me completely happy with the account you sent
me of the double stars; but it vexes me more and more that in this
abominable city there is no one who is capable of partaking in the
joy I feel on this revival of your father’s name. His observations on
double stars were, from first to last, the most interesting subject; he
never lost sight of it. And I cannot help lamenting that he could not
take to his grave the satisfaction I feel at seeing his son doing him
such ample justice by endeavouring to perfect what he could only begin.”

Sir John’s trip to the Cape roused her ardent sympathy. “Ja!” she
exclaimed, on hearing of the project, “If I were thirty or forty years
younger, and could go too. In Gottes Namen!” But she was eighty-two,
and could only give vent to her feelings by “jingling glasses
with Betty” after dinner on his birthday, while mistress and maid
together cried, “Es lebe Sir John! Hoch! Hurrah!” The reports of his
achievements in the southern hemisphere were, she said, “like a drop
of oil supplying my expiring lamp.” “At first, on reading them,” she
wrote to Lady Herschel, “I could turn wild; but this is only a flash;
for soon I fall into a reverie on what my dear nephew’s father would
have felt if such letters could have been directed to him, and cannot
suppress my wish that _his_ life instead of _mine_ had been spared
until this present moment.”

The joyful intelligence of her nephew’s safe return to England was
sent to Miss Herschel by the Duke of Cambridge, whose attentions to
her were unfailing; and she lived to hold in her hands the volume of
“Cape Results,” by which her brother’s great survey of the heavens
was rounded off to completion. But by that time the lassitude of
approaching death was upon her.

Three visits from her nephew broke the monotony of separation. In
October, 1824, he stopped at Hanover on his way homeward from the
Continent. Before his arrival, her “arms were longing to receive him”;
after his departure, she “followed him in idea every inch he moved
farther” away from her. Six years passed, and then he came again.

“I found my aunt,” he reported, June 19th, 1832, “wonderfully well, and
very nicely and comfortably lodged, and we have since been on the full
trot. She runs about the town with me, and skips up her two flights of
stairs as light and fresh at least as some folks I could name who are
not a fourth part of her age. In the morning till eleven or twelve she
is dull and weary; but as the day advances she gains life, and is quite
‘fresh and funny’ at ten or eleven p.m., and sings old rhymes, nay,
even dances! to the great delight of all who see her.”

Their final meeting was in 1838, when Sir John’s Cape laurels were just
gathered; and he brought with him his eldest son, aged six. But the
old lady was terrified lest the child should come to harm; his food,
his sleep, his scramblings, his playthings, were all subjects of the
deepest anxiety. Then Sir John, desiring to spare her “the sadness of
farewell,” perpetrated a moonlight flitting, which left her dismayed
and desolate at the abrupt termination of the visit, and smarting
with the intolerable consciousness of opportunities lost for saying
what could now never be said. “All that passed,” she said, “was like
Sheridan’s Chapter of Accidents.” It was too much for her; she did not
desire the repetition of a pleasure rated at a price higher than she
could afford to pay. “I would not wish on any account,” she told Lady
Herschel in 1842, “to see either my nephew or you, my dear niece, again
in this world, for I could not endure the pain of parting once more;
but I trust I shall find and know you in the next.”

She lived habitually in the past, and found the present--as Mrs.
Knipping, Dietrich’s daughter said--“not only strange, but annoying.”
Sometimes she would rouse herself from a “melancholy lethargy” to spend
a few moments “in looking over my store of astronomical and other
memorandums of upwards of fifty years’ collecting, and destroying
all that might produce nonsense when coming through the hands of a
Block-kopf into the Zeitungen.” Again she would dip back into the
career of the “forty-foot,” or recall the choral performance to
which the tube had resounded not far from sixty years before, “when
I was one of the nimblest and foremost to get in and out of it. But
now--lack-a-day--I can hardly cross the room without help. But what of
that? Dorcas, in the _Beggars’ Opera_, says:

    “‘One cannot eat one’s cake and have it too!’”

That venerable instrument marked for her the _ne plus ultra_ of optical
achievement. She would not admit the sacrilegious thought of its being
outdone. “I believe I have water on my brains,” she informed her nephew
in August, 1842, “and all my bones ache so that I can hardly crawl;
and, besides, sometimes a whole week passes without anybody coming
near me, till they stumble on a paragraph in the newspaper about
Gruithuisen’s discoveries, or Lord Queenstown’s great telescope, which
_shall_ beat Sir William Herschel’s all to nothing; and such a visit
sometimes makes me merry for a whole day.”

From time to time she wrote books of “Recollections,” which she
forwarded, with anxious care, to England. They contain nearly all that
is intimately known of Sir William Herschel’s life. The entries in her
“Day-book” ceased finally only on September 3rd, 1845. In the hope of
giving permanent form to the memories that haunted her, she began, at
ninety-two, “a piece of work which I despair of finishing before my
eyesight and life leave me in the lurch. You will, perhaps, wonder what
such a thing can be as I may pretend to do; but I cannot help it, and
shall not rest till I have wrote the history of the Herschels.” “You
remember,” she added, “you take the work in whatever state I may leave
it, and make the best of it at your leisure.” It remained a piquant
fragment. The fervour of her start was soon quenched by physical
collapse, and she acknowledged her powerlessness “to do anything beside
keeping herself alive.” Her last letter to Collingwood was finished
with difficulty, December 3rd, 1846. Monthly reports of her state,
however, continued to be sent thither by Miss Beckedorff, who, with
Mrs. Knipping, cared for her to the last.

In honour of her ninety-sixth birthday, the King of Prussia sent her,
through Humboldt’s friendly hands, the Gold Medal of Science; and on
the following anniversary, March 16th, 1847, she entertained the Crown
Prince and Princess for two hours. Not only with conversation; she
sang to them, too, a composition of Sir William’s, “Suppose we sing a
Catch.” She had a new gown and smart cap for the occasion; and seemed
“more revived than exhausted” by her efforts. Her last message to her
nephew and his family--sent March 31st--was to say, with her “best
love” “that she often wished to be with them, often felt alone, did not
quite like old age with its weaknesses and infirmities, but that she,
too, sometimes laughed at the world, liked her meals, and was satisfied
with Betty’s services.”

On the 9th of January, 1848, she tranquilly breathed her last, and “the
unquiet heart was at rest.” She was buried beside her parents in the
churchyard of the Gartengemeinde, at Hanover, with an epitaph of her
own composition.[F] It records that the eyes closed in death had in
life been turned towards the “starry heavens,” as her discoveries of
comets, and her participation in her brother’s “immortal labours,” bear
witness to future ages. By her special request a lock of “her revered
brother’s” hair, and an old almanac used by her father, were placed in
her coffin, which was escorted to the grave by royal carriages, and
covered with wreaths of laurel and cypress from the royal gardens at
Herrenhausen.

    [F] “Der Blick der Verklärten war hienieden dem gestirnten
        Himmel zugewandt; die eigenen Cometen-Entdeckungen,
        und die Theilnahme an den unsterblichen Arbeiten ihres
        Bruders, Wilhelm Herschel, zeugen davon bis in die späteste
        Nachwelt.”

Caroline Herschel was not a woman of genius. Her mind was sound and
vigorous, rather than brilliant. No abstract enthusiasm inspired her;
no line of inquiry attracted her; she seems to have remained ignorant
even of the subsequent history of her own comets. She prized them as
trophies, but not unduly. The assignment of property in comets reminded
her, she humorously remarked, when in her ninety-third year, of the
children’s game, “He who first cries ‘Kick!’ shall have the apple.”
Yet her faculties were of no common order, and they were rendered
serviceable by moral strength and absolute devotedness. Her persistence
was indomitable, her zeal was tempered by good sense; her endurance,
courage, docility, and self-forgetfulness went to the limits of what
is possible to human nature. With her readiness of hand and eye, her
precision, her rapidity, her prompt obedience to a word or glance, she
realised the ideal of what an assistant should be.

Herself and her performances she held in small esteem. Compliments and
honours had no inflating effect upon her. Indeed, she deprecated them,
lest they should tend to diminish her brother’s glory. “Saying too
much of what I have done,” she wrote in 1826, “is saying too little
of him, for he did all. I was a mere tool which _he_ had the trouble
of sharpening and adapting for the purpose he wanted it, for lack of
a better. A little praise is very comforting, and I feel confident
of having deserved it for my patience and perseverance, but none for
great abilities or knowledge.” Again: “I did nothing for my brother but
what a well-trained puppy-dog would have done; that is to say, I did
what he commanded me.” And her entire and touching humility appears
concentrated in the following sentence from a letter to her nephew: “My
only reason for saying so much of myself is to show with what miserable
assistance your father made shift to obtain the means of exploring the
heavens.”

The aim in life of this admirable woman was not to become learned
or famous, but to make herself useful. Her function was, in her own
unvarying opinion, a strictly secondary one. She had no ambition.
Distinctions came to her unsought and incidentally. She was accordingly
content with the slight and fragmentary supply of knowledge sufficing
for the accurate performance of her daily tasks. No inner craving
tormented her into amplifying it. The following of any such impulse
would probably have impaired, rather than improved, her efficiency.
The turn of her mind was, above all things, practical. She used
formulæ as other women use pins, needles and scissors, for certain
definite purposes, but with complete indifference as to the mode of
their manufacture. What was required of her, however, she accomplished
superlatively well, and this was the summit of her desires. She shines,
and will continue to shine, by the reflected light that she loved.




CHAPTER VII.

SIR JOHN HERSCHEL AT CAMBRIDGE AND SLOUGH.


“The little boy is entertaining, comical, and promising,” Dr. Burney
wrote after his visit to Slough in 1797. John Frederick William
Herschel was then five years old, having been born “within the shadow
of the great telescope” March 7, 1792. He was an industrious little
fellow, especially in doing mischief. “When one day I was sitting
beside him,” his aunt relates, “listening to his prattle, my attention
was drawn by his hammering to see what he might be about, and I found
that it was the continuation of many days’ labour, and that the ground
about the corner of the house was undermined, the corner-stone entirely
away, and he was hard at work going on with the next. I gave the alarm,
and old John Wiltshire, a favourite carpenter, came running, crying
out, ‘God bless the boy, if he is not going to pull the house down!’”
And she wrote to him at Feldhausen; “I see you now in idea, running
about in petticoats among your father’s carpenters, working with little
tools of your own, and John Wiltshire crying out, ‘Dang the boy, if he
can’t drive in a nail as well as I can!’”

[Illustration: SIR JOHN FREDERICK WILLIAM HERSCHEL, BART.

(_From a portrait painted by Pickersgill for St. John’s College,
Cambridge._)]

“John and I,” she told his wife, “were the most affectionate friends,
and many a half or whole holiday spent with me was dedicated to making
experiments in chemistry, in which generally all boxes, tops of
tea-canisters, pepper-boxes, teacups, etc., served for the necessary
vessels, and the sand-tub furnished the matter to be analysed. I only
had to take care to exclude water, which would have produced havoc on
my carpet.”

From a preparatory school kept by Dr. Gretton at Hitcham, he was sent,
a delicate, blue-eyed lad, to Eton. His mother, however, happening to
see him maltreated by a stronger boy, brought him home after a few
months, and his education was continued by a Scotch mathematician named
Rogers, a man of considerable ability. His pupil held him in high
respect; yet, though he learned Euclid accurately from him, he told
Dr. Pritchard afterwards that “he knew no more of its real bearing and
intention than he knew of the man in the moon.” The results of the home
tuition were, none the less, exceedingly brilliant.

Herschel entered St. John’s College, Cambridge, at the age of
seventeen, and his aunt noted in her Diary that, from the time of his
admittance to the University until he quitted it, he gained all the
first prizes without exception. He graduated as Senior Wrangler and
First Smith’s Prizeman in 1813, a year in which honours were not cheap.
Peacock, subsequently Dean of Ely, took second place, Fearon Fallows,
the first Royal Astronomer at the Cape of Good Hope, came third, and
Babbage withdrew from the competition, judging himself unable to beat,
and not caring to be beaten by Herschel. Rivalry did not disturb their
friendship. Having entered, together with Peacock, into a juvenile
compact to do what in them lay “to leave the world wiser than they
found it,” they, in 1812, set about fulfilling it by the establishment
of the “Analytical Society of Cambridge.” Its object was to substitute
in England for Newton’s fluxional method the more flexible and powerful
calculus in use on the Continent; or, as Babbage expressed it, punning
on the required change of notation, “to uphold the principles of pure
D-ism in opposition to the _Dot_-age of the University.” The trio of
innovators were full of enthusiasm, and they carried through a reform
vital to the progress of British science. Herschel laboured zealously
in the cause. In combination with his two allies, he translated
Lacroix’s elementary treatise on the Differential Calculus, which
became a text-book at Cambridge; and published, in 1820, an admirable
volume of “Examples.” “In a very few years,” to use Babbage’s words,
“the change from dots to d’s was accomplished; and thus at last the
English cultivators of mathematical science, untrammelled by a limited
and imperfect system of signs, entered on equal terms into competition
with their Continental rivals.” Herschel, writing in the _Quarterly
Review_, playfully described the process by which this was brought
about. “The brows of many a Cambridge moderator,” he said, “were
elevated, half in ire, half in admiration, at the unusual answers which
began to appear in examination-papers. Even moderators are not made
of impenetrable stuff; their souls were touched, though fenced with
seven-fold Jacquier, and tough bull-hide of Vince and Wood. They were
carried away with the stream, in short, or replaced by successors full
of their newly acquired powers. The modern analysis was adopted in its
largest extent.”

John Herschel was one of Babbage’s “chief and choicest companions,” who
breakfasted with him every Sunday after chapel, and discussed, during
three or four delightful hours, “all knowable, and many unknowable
things.” His life-long friendship with Whewell began after his election
to a Fellowship of his College. It lent charm to the occasional
residences at Cambridge, which terminated in 1816, on his attaining the
dignity of Master of Arts. He celebrated his coming of age at home,
and was with his father at Brighton when Campbell characterised him as
“a prodigy in science, and fond of poetry, but very unassuming.” His
first publication was a paper on “Cotes’s Theorem,” sent, in October,
1812, to the Royal Society, of which body he was chosen a member, May
27, 1813. This was followed by a series of memoirs on various points
of analysis, their signal merit being recognised, in 1821, by the
bestowal of the Copley Medal. His investigations in pure mathematics
were carried no further; but he had done enough to show his power and
originality, and materially to widen the scope of the new methods.

He was in no hurry to choose a profession. Evenly balanced inclinations
demanded, circumstances indulged delay; so he paused. His father wished
him to enter the Church; but he preferred the law, and was enrolled
a student at Lincoln’s Inn, January 24, 1814. The step was a simple
formality. It committed him to nothing. And, in fact, while nominally
reading for the Bar, his thoughts were running in a totally different
direction. Dr. Wollaston, whose acquaintance he made in London,
fascinated him, and his influence served to steady the helm of his
intentions. Having decided finally for a scientific career, he returned
to Slough, and plunged into experiments in chemistry and physical
optics.

On September 10th, 1816, he informed a correspondent that he was
“going, under his father’s direction, to take up star-gazing.” This
brief sentence gives the first tidings of an astronomical element in
his life. Its growth was slow. He had no instinctive turn that way. It
was through filial reverence that he resolved to tread in his father’s
footsteps. His self-denial received a magnificent reward. He took a
place expressly reserved for him, as it might seem, beside his father
as an explorer of the skies on the grandest scale. But for this moral
purpose, he might have squandered time in a multiplicity of partial
researches. So late as 1830 he told Sir William Rowan Hamilton: “I find
it impossible to dwell for very long on one subject, and this renders
my pursuit of any branch of science necessarily very desultory.” His
nebulæ and double stars saved him from being “everything by turns,
and nothing long.” Their collection and revisal, begun as a duty,
grew to be irresistibly attractive, and John Herschel pledged himself
definitively to astronomy.

His earliest undertaking was the re-examination of his father’s
double stars. Entered upon at Slough in 1816, it was continued from
1821 to 1823 at the observatory in Blackman Street, Southwark, of
Mr., afterwards Sir James South, where, with two excellent refracting
telescopes, of five and seven feet focal length, the colleagues
measured 380 of Sir William Herschel’s original pairs. Double stars
want a great deal of looking after. Their discovery should be the
prelude to long processes of investigation. It is of little interest
unless diligently followed up. Each represents a system, individual
in its peculiarities, and probably of most complex organisation.
The more such systems are studied, the more wonderful they appear.
Two associated stars have often proved, on keener scrutiny, to be
themselves very closely double; and in other cases, disturbed motion
has revealed the existence of obscure masses--planets on a colossal
scale, possibly the spacious abodes of unimaginable forms of life.

The “Astronomy of the Invisible,” however, was still in the future when
Herschel and South did their work. Facts relating to binary revolutions
were scantily forthcoming, and the science to be founded on them had
been rather indicated than established. Fresh observations were then
needed to ascertain how the circling stars had behaved since 1802. The
results proved highly satisfactory. In Francis Baily’s words, “The
remarkable phenomena first brought to light by Sir William Herschel
were abundantly confirmed, and many new objects pointed out as worthy
the attention of future observers.” To take a couple of examples. Eta
Coronæ was found to have described, since 1781, one entire round,
and to be just starting on a second. Again, Tau Ophiuchi had been
perceived, by the elder Herschel, at his first sight of it in April,
1783, to be “elongated.” “One half of the small star,” he said, “if
not three-quarters, seems to be behind the large star.” This effect
was imperceptible to his son. It had become entirely effaced in the
course of forty years. The star was, in 1823, perfectly round; it had,
as it were, absorbed its companion. By slow degrees, however, the two
came into separate view, and now form an easy telescopic object. Their
period of revolution is not less than two centuries. Another point of
special interest was the detection of marked eccentricity in a stellar
orbit--that of Xi Ursæ Majoris. These stars perform their circuits in
just sixty years; but in 1821 their apparent speed was so great that
changes in their relative positions could be determined from month to
month. For these observations, published with notes and discussions in
the _Philosophical Transactions_ for 1824, Herschel and South received
the Lalande Prize of the French Academy in 1825, and the Gold Medal of
the Astronomical Society in 1826. In the latter distinction, Wilhelm
Struve and Amici of Modena were associated with them. These four were
the only double star observers then living.

Their exertions served to define more closely the circumstances of
stellar movement. The crucial question could now be put, whether they
are governed by the force that binds the planets to the sun, or by
some other form of attractive influence. In other words, is the law of
gravitation universal? An answer could only be obtained experimentally,
by computing, on gravitational principles, the paths of the best-known
pairs, and then _trying the fit_. If the stars, as time went on, kept
near their predicted places, the unity of nature in this respect might
be safely inferred; although considerable discrepancies might in any
case be expected, owing to errors of measurement minute in themselves,
but large relatively to curves reduced by distance to hair-breadth
dimensions.

This kind of inquiry was fairly started in 1827, when Savary computed
the orbit of Xi Ursæ. His success made it almost certain that the pair
moved under the planetary regimen, conformed to, there is no reason
to doubt, by all binaries. John Herschel, although not the first, was
the most effective early investigator of stellar orbits. His method,
described before the Royal Astronomical Society January 13, 1832, and
approved by the award of its Gold Medal in 1833, went to the root of
the matter. The author declared it a mere waste of time to attempt to
deal, by any refined or intricate process of calculation, with data so
uncertain and irregular as those at hand. “Uncertain and irregular,”
it must be repeated, because referred to a scale on which tenths of
a second assume large proportions. He accordingly discarded, as mere
pedantic trifling, such analytical formulæ as those employed by Savary
and Encke, and had recourse to a graphical process, in which “the
aid of the eye and hand” was used to “guide the judgment in a case
where judgment only, and not calculation, could be of any avail.” The
operation which he went on to explain was commended by Sir George Airy
for its “elegance and practical utility.” Nothing more appropriate
could have been devised than this plan, at once simple, ingenious, and
accommodating, for drawing a curve representative of the successive
relative positions of double stars. Its invention effectively promoted
acquaintance with their orbits; most of those at present known having,
indeed, been calculated with its aid.

In 1821, Herschel travelled, in Babbage’s company, through Switzerland
and Italy. His only recorded adventure was an ascent of Monte Rosa.
In the following year he visited Holland with James Grahame, the
learned author of a “History of America”; and on the removal of
South’s observatory to Passy, he again went abroad, starting with
Babbage, but returning alone. This time he made a number of scientific
acquaintances. His father’s name worked like a spell. “I find myself,”
he said, “for his sake, received by all men of science with open arms.”
His modesty forbade him to remember that his own merits were already
conspicuous. In Paris, Arago and Fourier showed him all possible
attentions; he was welcomed at Turin “like a brother” by Plana, “one
of the most eminent mathematicians of the age;” at Modena, Amici was,
if possible, still more cordial. “He is the only man,” Herschel told
his aunt, “who has, since my father, bestowed great pains on the
construction of specula.” “Among other of your inquiring friends,” he
continued, “I should not omit the Abbé Piazzi, whom I found ill in
bed at Palermo, and who is a fine, respectable old man, though, I am
afraid, not much longer for this world. He remembered you personally,
having himself visited Slough.”

On July 3 Herschel “made the ascent of Etna, without particular
difficulty, though with excessive fatigue.” On the summit, reached
before sunrise, by “a desperate scramble up a cone of lava and ashes,
one thousand feet high,” he found himself “enveloped in suffocating
sulphurous vapours”; and “was glad enough to get down,” after having
made a reading of the barometer in concert with the simultaneous
observations of the brothers Gemellaro at Catania and Nicolosi. The
same night he arrived at Catania “almost dead” from the morning’s
arduous climb, “and the dreadful descent of nearly thirty miles, where
the mules could scarce keep their feet.”

In traversing Germany, he deviated to Erlangen, where Pfaff was
engaged in translating Sir William Herschel’s writings; and visited
Encke, Lindenau, and Harding, at Seeberg, Gotha, and Göttingen. With
Göttingen he had a special tie through his creation, in 1816, an
honorary member of the University; and at Göttingen, too, he hoped to
meet Gauss--a man of strange, and--to the lay mind--unintelligible
powers. “Gauss was a god,” one of his fellow-mathematicians said of
him; but the “god” was on this occasion absent--feasting with the
“blameless Ethiopians,” perhaps, like the Homeric deities when wanted.
He was reported “inconsolable” for the lost opportunity, which seems
never to have recurred.

From Munich Herschel wrote to his aunt, in view of his approaching
visit to Hanover:--“I hope you haven’t forgotten your English, as
I find myself not quite so fluent in this language (German) as I
expected. In fact, since leaving Italy, I have so begarbled my German
with Italian that it is unintelligible both to myself and to everyone
that hears it: and what is very perverse, though when in Italy I could
hardly talk Italian fit to be heard, I can now talk nothing else, and
whenever I want a German word, pop comes the Italian one in its place.
I made the waiter to-day stare (he being a Frenchman) by calling to
him, ‘Wollen Sie avere la bontà den acet zu apportaren!’ But this, I
hope, will soon wear off.”

His next foreign holiday was spent in France. He had designed a new
instrument for measuring the intensity of the sun’s radiations, and
was eager to experiment with it alternately at high and low levels,
for the purpose of determining the proportion of solar heat absorbed
by the earth’s atmosphere. This method was employed with fine effect
by Professor Langley on Mount Whitney in 1881. Herschel carried his
“actinometer” to the top of the Puy de Dôme in September 1826, and
waited at Montpellier for “one day of intense sunshine,” in order
to procure his second term of comparison. The Puy de Dôme, with its
associated three hundred summits, strongly allured him. “I have been
rambling over the volcanoes of Auvergne,” he wrote from Montpellier,
September 17, “and propose, before I quit this, to visit an extinct
crater which has given off two streams of lava at Agde, a town about
thirty miles south of this place on the road to the Spanish frontier.
Into Spain, however, I do not mean to go--having no wish to have my
throat cut. I am told that a regular diligence runs between this and
Madrid, and is as regularly stopped and robbed on the way.”

This exploratory turn alarmed Miss Herschel. “I fear,” she replied,
“you must often be exposed to great dangers by creeping about in holes
and corners among craters of volcanoes.” He was, nevertheless, only
dissuaded by his mother’s anxious remonstrances from pursuing their
study in Madeira and Teneriffe.

In the autumn of 1827, Babbage accompanied him to Ireland. The young
Astronomer Royal, Sir W. R. Hamilton, was unluckily absent at the time
of their visit; but he sent Herschel, by way of compensation, one of
his brilliant optical essays, and a correspondence sprang up from which
a lasting friendship developed.

Herschel’s scientific occupations at home were meanwhile various and
pressing. He co-operated in the foundation of the Astronomical Society,
and became in 1821 its first foreign secretary. In 1824 he undertook
the more onerous duties of secretary to the Royal Society, and rented a
house in Devonshire Street for the three years of his term of office.
Astronomy, it might have been feared, should be at least temporarily
shelved; yet he informed his aunt, April 18, 1825, “A week ago I had
the twenty-foot directed on the nebulæ in Virgo, and determined the
right ascensions and polar distances of thirty-six of them. These
curious objects I shall now take into my especial charge--nobody else
can see them.”

His telescope, in fact, then held the championship. It was constructed
in 1820 by himself, under his father’s directions, on the “front view”
plan, the speculum being eighteen inches in diameter, and of twenty
feet focal length. With it he executed, in 1824, a fine drawing of the
Orion Nebula, with which “inexplicable phenomenon” he was profoundly
impressed. It suggested to him no idea of a starry composition, and he
likened its aspect to that presented by the “breaking up of a mackerel
sky, when the clouds of which it consists begin to assume a cirrous
appearance.”

In July, 1828, he succeeded in discerning the two Uranian satellites,
Oberon and Titania, _authentically_ discovered by his father. They had
not been seen, except incidentally at Slough, for thirty years. His
pursuit of them, continued at intervals until 1832, had the result
of confirming, while slightly correcting, Sir William Herschel’s
elements of their motions. On September 23, 1832, he perceived Biela’s
comet as a round, hazy object without a tail. It closely simulated a
pretty large nebula. A small knot of very faint stars lay directly
in its path, and, having before long overtaken them, it “presented,
when on the cluster, the appearance of a nebula partly resolved into
stars, the stars of the cluster being visible through the comet.” They
shone undimmed, he estimated, from behind a veil of cometary matter
50,000 miles thick. Yet, only a month later, the remote prospect of a
collision with this tenuous body threw Europe into a panic.

After Sir William Herschel’s death, his son formed the project of
collecting into a memorial volume all his published papers; but he
decided before long that he could add more to his fame by pursuing
and verifying his observations than by reprinting them. The keynote
of his life’s activity was struck in these words. His review of the
2,500 Herschelian nebulæ, more than half of which were invisible with
any instrument except his own, was begun in the summer of 1825, and
terminated in 1833. The assiduity with which it was prosecuted appeared
by its completion in little more than half the time judged necessary
for the purpose by the original discoverer. Yet he was not exempt
from discouragement. “Two stars last night,” he wrote, July 23, 1830,
“and sat up till two waiting for them. Ditto the night before. Sick
of star-gazing--mean to break the telescopes and melt the mirrors.”
Very few glimpses of this seamy side to the occupation are afforded us
by either of the Slough observers. Modern astronomers, by comparison,
would seem, like the Scotchman’s barometer, to have “lost all control
over the weather.”

The efficacious promptitude with which John Herschel swept the skies
appears truly wonderful when we remember that he was without a skilled
assistant. No ready pen was at hand to record what he saw, and how
he saw it; he was, by necessity, his own amanuensis; and writing by
lamplight unfits the eye for receiving delicate impressions. Yet a
multitude of the objects for which quest was being made were of the
last degree of faintness. The results were none the less admirable.
Embodied in a catalogue of 2,307 nebulæ, of which 525 were new, they
were presented to the Royal Society July 1, 1833, and printed in the
_Philosophical Transactions_ (vol. cxxiii.). Annotations of great
interest, and over one hundred beautiful drawings, enhanced the value
of the memoir.

Herschel was struck, in the course of his review, by the nebulous
relations of double stars. A close, faint pair at the exact centre of
a small round nebula in Leo; stellar foci in nebular ellipses; and a
strange little group consisting of a trio of equidistant stars relieved
against a nebulous shield, were specimen-instances illustrating “a
point of curious and high physical interest.”

He also drew attention to “the frequent and close proximity to
planetary nebulæ of minute stars which suggest the idea of accompanying
satellites. Such they may possibly be.” If so, their revolutions might
eventually be ascertained; and he urged the desirability of exact and
persistent determinations of the positions of these satellite-stars.
“I regret,” he concluded, “not having sufficiently attended to this in
my observations, the few measures given being hurried, imperfect, and
discordant.” Up to the present, these supposed systems have remained
sensibly fixed; but they have been a good deal neglected. Mr. Burnham’s
observations, however, with the Lick refractor in 1890–1, may supply a
basis for the future detection of their movements in periods probably
to be reckoned by millenniums.

The orbital circulation of compound nebulæ must be at least equally
slow. They are most diverse in form and arrangement. “All the varieties
of double stars as to distance, position, and relative brightness,”
Herschel wrote, “have their counterparts in nebulæ; besides which, the
varieties of form and gradation of light in the latter afford room for
combinations peculiar to this class of objects.” Such, for instance, as
the disparate union of an immensely long nebulous ray in Canes Venatici
with a dim round companion, a small intermediate star occupying
possibly the centre of gravity of the system.

Herschel’s drawings of double nebulæ have gained significance through
their discussion, in 1892, by Dr. T. J. J. See of Chicago. They are
now perceived to form a series aptly illustrative of the process,
theoretically investigated by Poincaré and Darwin, by which a cooling
and contracting body, under the stress of its consequently accelerated
rotation, divides into two. If it be homogeneous in composition,
its “fission” gives rise to two equal masses, presumed to condense
eventually into a pair of equal stars. Disparity, on the other hand,
between the products of fission indicates original heterogeneity;
so that a large nebula must be of denser consistence than a smaller
one physically connected with it. The chemical dissimilarity of the
stars developed from them might explain the colour-contrasts often
presented by unequal stellar couples. This view as to the origin of
double nebulæ, and through them of double stars, although doubtless
representing only a fragment of the truth, gives wonderful coherence to
Herschel’s faithful delineations of what his telescope showed him.

No one before him had completely seen the “Dumb-bell” nebula in
Vulpecula. Sir William Herschel had perceived the “double-headed shot”
part of this “most amazing object,” but had missed the hazy sheath
which his successor noticed as filling in the elliptic outline. He
perceived similarly (unaware of Schröter’s observation) that the
interior of the Ring-nebula in Lyra is not entirely dark; and compared
the effect to that of fine gauze stretched over a hoop. An exceedingly
long, nebular ellipse in Andromeda, with a narrow interior vacuity,
left him “hardly a doubt of its being a thin, flat ring of enormous
dimensions, seen very obliquely.” A photograph taken by Dr. Roberts, in
1891, corresponds strikingly with Herschel’s drawing. Some specimens of
“rifted nebulæ,” were also included in the collection of 1833. They are
double or even triple parallel rays, fragments, apparently, of single
primitive formations. Herschel might well assert that “some of the most
remarkable peculiarities of nebulæ had escaped every former observer.”

Both by the Royal, and by the Royal Astronomical Societies, medals
were, in 1836, adjudged to this fine work. Its progress was
accompanied by the discovery of 3,347 double stars, as well as by the
re-measurement of a large number of pairs already known. The whole
were drawn up into eight catalogues, presented at intervals to the
Astronomical Society, and printed in their Memoirs. A good many of
them would, nevertheless, be rejected by modern astronomers as “not
worth powder and shot,” the stars composing them being too far apart to
give more than an infinitesimal chance of mutual connection. From May
1828 onwards, these measures were made with “South’s _ci-devant_ great
equatorial,” purchased by Herschel. The object-glass, by Tulley, was
five inches in diameter. With a twelve-inch refractor, its successor
in South’s observatory on Campden Hill, Herschel detected, on its
trial-night, February 13, 1830, the sixth star in the “trapezium” of
Orion. This minute object was then about one-third as bright as the
fifth star in the same group, discovered by Robert Hooke in 1664, but
forgotten, and re-discovered by Struve in 1826. A slow gain of light in
Herschel’s star is not improbable.

He refused, in 1826, to compete for the Lucasian Professorship of
Mathematics at Cambridge. It was practically at his disposal, since all
agreed that no one could better than Herschel have filled the chair
once occupied by Newton. He was, however, disinclined for an University
career, and had undertaken labours incompatible with it. In 1830 he
stood as the “scientific candidate” for the presidentship of the Royal
Society, against the Duke of Sussex. His defeat was by “a ridiculously
small majority.” “I had no personal interest in the contest,” he
wrote to Sir William Hamilton. “Had my private wishes and sense of
individual advantage weighed with me in opposition to what, under the
circumstances, was an imperative duty, I should have persisted in my
refusal to be brought forward; but there are situations where one _has_
no choice, and such was mine.”

He made Hamilton’s personal acquaintance at a dinner of notabilities,
given by the Duke of Sussex, in March, 1832. An invitation to Slough
followed, and Hamilton, arriving “in a beautiful star-time,” enjoyed
celestial sights that seemed the opening of a new firmament.

Herschel married, March 3, 1829, Margaret Brodie, second daughter of
the Rev. Alexander Stewart, of Dingwall, in Ross-shire. The event--not
merely by convention a “happy” one--gave great satisfaction to his
numerous friends. Miss Herschel was beside herself with glad emotion.
“I have spent four days,” she informed him on his wedding-day, “in
vain endeavours to gain composure enough to give you an idea of the
joyful sensation caused by the news. But I can at this moment find no
words which would better express my happiness than those of Simeon:
“Lord, now lettest thou thy servant depart in peace.” But there was
no finality in her desires for this brilliant scion of her race.
His domestic felicity did not long content her; she craved worldly
distinctions. When, after the accession of William IV., a shower of
honours was let fall, she began to think plain “John Herschel, Esq.,”
an address very inadequate to his merits. “Dr. Grosskopf,” the husband
of one of her nieces, “has been _zum Ritter ernannt_ by his present
Majesty,” she wrote discontentedly. “So was Dr. Mükry last week. If all
is betitled in England and Germany, why is not my nephew, J. H., a lord
or a wycount (_sic_) at least? General Komarzewsky used to say to your
father, ‘Why does not King George III. make you Duke of Slough?’”

An instalment of her wishes was granted by his creation, in 1831, a
Knight of the Royal Hanoverian Guelphic Order; and she lived to see him
a baronet. She had no inkling of his approaching journey to the Cape
when he came to see her in June, 1832, although the visit was designed
as a farewell. Hanover itself, too, had for him an ancestral charm.

“It was only this evening,” he wrote home, “that, escaping from a
party at Mrs. Beckedorff’s, I was able to indulge in what my soul has
been yearning for ever since I came here--a solitary ramble out of
town, among the meadows which border the Leine-strom, from which the
old, tall, sombre-looking Marktthurm, and the three beautiful lanthorn
steeples of Hanover are seen as in the little picture I have often
looked at with a sort of mysterious wonder when a boy, as that strange
place in foreign parts that my father and uncle used to talk so much
about, and so familiarly. The _likeness_ is correct, and I soon found
the point of view.”

Almost from the beginning of his surveying operations, Herschel
cherished the hope of extending them to the southern hemisphere. But
during his mother’s lifetime, he took no steps towards its realisation.
The separation would have been cruel. Her death, however, on January
6th, 1832, at the age of eighty-one, removed this obstacle, and
the scheme rapidly took shape. The station originally thought of
was Parramatta, in New South Wales; but Dunlop’s observations there
anticipated him, and he reflected with disappointment that “the cream
of the southern hemisphere had been skimmed” before his turn came. He
learned afterwards that nothing important in the “sweeping” line had
been done at Parramatta; he had virgin skies to explore. A trip to the
Himalayas was his next ambition; and one of the recommendations of the
Cape of Good Hope was its being “within striking distance of India.”
But to India he never went. The Cape was beyond question the most
suitable locality for his purpose, and it would have been waste of time
to have left it, even temporarily, for any other. He was offered a free
passage thither in a ship of war, but preferred to keep his enterprise
altogether on a private footing. So having embarked with his wife,
three children, and instrumental outfit, on board the _Mountstuart
Elphinstone_, he left the shores of England, November 13, 1833.




CHAPTER VIII.

EXPEDITION TO THE CAPE.


The voyage was prosperous, but long. Nine weeks and two days passed
before the welcome cry of “Land” was heard; and it was in the dawn
of January 15, 1835, that Table Mountain at last stood full in view,
“with all its attendant range down to the farthest point of South
Africa,” outlined, ghost-like, in clear blue. The disembarkation of the
instruments and luggage took several days. They filled fifteen large
boats, and a single onslaught of the south-easterly gale, by which at
that time of the year Cape Town is harried, might easily have marred
the projected campaign. All, however, went well.

The travellers were welcomed by Dr. Stewart, one of Lady Herschel’s
brothers, and enthusiastically greeted by the Royal Astronomer, Sir
Thomas Maclear. They made no delay in fixing their headquarters.

“For the last two or three days,” Herschel wrote to his aunt, January
21, “we have been looking for houses, and have all but agreed for one,
a most beautiful place four or five miles out of town, called ‘The
Grove.’ In point of situation it is a perfect paradise in rich and
magnificent mountain scenery, and sheltered from all winds, even the
fierce south-easter, by thick surrounding woods. I must reserve for my
next all description of the gorgeous display of flowers which adorns
this splendid country, as well as the astonishing brilliancy of the
constellations.”

“The Grove” resumed its old Dutch name of “Feldhausen” during
Herschel’s occupation of it; and as “Feldhausen” it will always
be memorable in astronomical history as the scene of the first
effective exploration of the southern heavens. The place is
essentially unchanged. Only an avenue of fir-trees has been planted
by way of approach to the house, a solid Dutch structure, with a
disconsolate-looking garden in front; while in an adjacent field,
carpeted with yellow lupins every spring, and redolent of their
perfume, an obelisk has been erected on the former site of the great
reflector. Above, to the west, towers the _gable-end_ of Table
Mountain, and an exuberant growth of oaks and pines softens the
sternness of its “mural precipices.”

The neighbourhood was, in those days, lonely in the human sense,
although otherwise over- and ill-populated. Wolves and jackals abounded
in the forests; venomous snakes slid through the grass; baboons had the
run of the country; even the lion and the hippopotamus were scarcely
yet extinct in the Cape Peninsula. Many a wild hyæna-shriek startled
the astronomer at his nightly toil; and Dr. Whewell reported that he
had “spent one night in tiger-hunting, but seemed to think it poor
sport compared with the _chasse aux étoiles doubles_.” _Tiger_, it
should be explained, is a local name for a species of leopard: no true
tigers have ever been encountered in Africa.

His twenty-foot began its activity February 22nd, and the refractor,
which was equatorially mounted in a revolving dome, was ready early
in June. “But I am sorry to say,” he told Miss Herschel, “that the
nights in which it can be used to advantage are rare.” And he lamented
to his brother-in-law and intimate friend, Mr. James C. Stewart,
that, during the hot season, “the stars tremble, swell, and waver most
formidably.” The Cape heavens are indeed often exasperating. On nights
meteorologically quite fine, the dismayed astronomer not uncommonly
sees the stars “walking about” in the field of view; and a mere handful
of cloud will, at other times, with incredible swiftness, spread over
the whole face of the sky. Still, compensation is, sooner or later,
sure to come in a run of magnificent observing weather. This was
Herschel’s experience. He informed Francis Baily, October 23rd, 1834,
that “the definition was far beyond anything experienced in England.”
After rain especially, superb opportunities were afforded, when

    “The starry sequence of nocturnal hours”[G]

    [G] R. Garnett, “Iphigenia in Delphi.”

might be unbroken, perhaps for a week together, by a single adverse
incident of climate.

Herschel took three specula with him to the Cape; one made by his
father, another by himself with his father’s aid, and a third, of his
own exclusive manufacture. Their rapid tarnishing kept them in constant
circulation from the tube to the polisher. After half a dozen nights
they had lost all brilliancy; at the end of three months, they were
more than purblind. He acquired, however, such facility and skill in
the use of his polishing machine, that he was able, in 1835, to report
his mirrors as “more perfect than at any former time.”

He made astonishingly quick progress in observation. On October 24th,
1835, Miss Herschel was informed, “I have now very nearly gone over
the whole southern heavens, and over much of it often. In short, I
have, to use a homely phrase, broken the neck of the work, and my main
object now is to secure and perfect what is done.”

His sweeps yielded a harvest of 1,202 double stars, and 1,708 nebulæ
and clusters, only 439 of which had been previously registered. Among
the novelties were a faint, delicate miniature of the ring-nebula
in Lyra, and five planetaries. One of these he described as “of a
beautiful greenish-blue colour, a full and intense tint.” This lovely
object, situated in Centaur, is sometimes distinguished as “_the_ blue
planetary”; although its hue is shared by all the members of its class.
The nature of their spectrum, in fact, obliges them to be more or less
green.

Sir John Herschel applied the term “falcated” to two curious nebulæ
belonging, undoubtedly, to the later recognised “spiral” class. He
perceived besides in oval nebulæ the annular lines of structure
emphasised in Dr. Roberts’s photographs. He remarked, further, that “as
the condensation increases toward the middle, the ellipticity of the
strata diminishes.”

His study of the Magellanic Clouds gave the first idea of their
composition. He showed them to be aggregations on a vast scale of
every variety of cosmical product. “When examined through powerful
telescopes, the constitution of the Nubeculæ, and especially of the
Nubecula Major, is found to be of astonishing complexity.” He drew up
a preliminary catalogue of 1,163 stars, nebulæ and clusters included
in them, the conjunction of which was really decisive as to nebular
status. For he showed, from the elementary principles of trigonometry,
that, taking the Greater Cloud to be roughly spherical in shape, its
nearest and remotest parts could differ in distance from ourselves
by little more than one-tenth the distance of its centre. The fact
was thus demonstrated that seventh and eighth-magnitude stars and
irresolvable nebulæ co-exist within those limits. He stopped short,
however, of the conclusion drawn by Whewell and Spencer, that the
stellar and nebular sub-kingdoms are not only locally intermixed, but
inseparably united.

The Magellanic Clouds are the most conspicuous features of the barren
south polar heavens. Round the Lesser Cloud especially, the sky,
Herschel said, “is most oppressively desolate.” And again: “The access
to the Nubecula Minor on all sides is through a desert.” One of the
separate inmates of the Larger Cloud is the “great looped nebula,”
compared by Herschel to “an assemblage of loops,” the complicated
windings of which make it “one of the most extraordinary objects which
the heavens present.” To the eye of the present writer it resembled
a shining strip of cellular tissue hung up against the sky. The
“lace-work nebula” in Cygnus is of the same type; but here the tracery
of nebula is closely followed by a tracery of stars. Truly, “A most
wonderful phenomenon!” as Herschel exclaimed in contemplating it.

The first photographs of the Magellanic Clouds were taken in 1890–91
by Mr. Russell of Sydney. They contained an extraordinary revelation.
Both objects came out in them as gigantic spirals. Their miscellaneous
contents are then arranged according to the dictates of a prevalent,
though unexplained cosmical law. The Nubecula Major is a double vortex,
and the extent of its outlying portions, invisible except to the
camera, is at least eight times that of the central mass; but they
conform to the same helical lines.

Herschel catalogued 1,203 stars strewn over the surface of the famous
Argo nebula, and devoted several months to its delineation. This he
found “a work of great labour and difficulty.” While at the telescope
he often half surrendered to despair “of ever being able to transfer to
paper, with even tolerable correctness, its endless details.” “Language
cannot easily convey,” he said, “a full impression of the beauty and
sublimity of the spectacle this nebula offers when viewed in a sweep,
ushered in by so glorious and innumerable a procession of stars, to
which it forms a sort of climax.” Only the Orion nebula may be thought
to surpass it in “magnitude, complexity, and brightness.” Its most
characteristic feature is an abrupt vacuity, of a “lemniscate oval”
shape, from which it derives the name of the “Keyhole Nebula.” The
value of Herschel’s drawing of this grand object has been accentuated
by its photographic portrayal. Their comparison betrays, in fact,
the occurrence in the interval of what appears to be a vast change.
Already, in 1871, Mr. Russell missed with surprise a prominent feature
in the Feldhausen picture; and its failure to appear on photographic
plates exposed for eight hours, yet impressed with innumerable stars
previously unseen, raised something more than a presumption that, as
Mr. Russell said, “a well-defined and brilliant portion of this nebula
vanished between 1837 and 1871.” Its disappearance was independently
verified by Dr. Gill, Royal Astronomer at the Cape. With a total
exposure of more than twelve hours, in March, 1892, he secured a
magnificent representation of this wonderful object, fundamentally
agreeing with Herschel’s, save only as regards the mass of bright
nebulosity vainly looked for by Mr. Russell. The “swan-shaped” or
“trident-like” structure was clean gone! That is to say, the matter
composing it had ceased to be luminous. It should be added that Mr.
Ranyard, whose special experience lent weight to his opinion, thought
it unsafe to trust much to comparisons of drawings of such baffling
objects, either among themselves or with photographs.

Before leaving the Cape, Herschel witnessed an event testifying
surprisingly to the _vitality_ of this nebula. In a condensed tract
close to the dark “keyhole,” he was accustomed to see the bright star
Eta Argûs. It gave no sign of being variable until, on December 16,
1837, he perceived with amazement that it had, all at once, nearly
tripled in brightness. After this sudden leap, it mounted gradually
to the level of Alpha Centauri, then slowly declined. It just matched
Aldebaran when Herschel lost sight of it in March, 1838. A second, and
even more vigorous outburst was watched by Sir Thomas Maclear in 1843.
It then overtopped every star except Sirius, and for seven subsequent
years rivalled the splendour of Canopus. No notice was at first taken
of its colour; but it was redder than Mars in 1850, and reddish it
still remains, in its low estate of invisibility to the naked eye. But
since bright lines of hydrogen show in its photographed spectrum, we
may suspect that--

    “Even in its ashes live its former fires,”

and that, consequently, its vicissitudes are not yet terminated. The
instability of its character was virtually discovered at Feldhausen.
Except by Burchell, the African traveller, no previous suspicion of
it had been entertained; the numerous facts denoting that the star’s
past behaviour had been abnormal were collected by Sir John Herschel
after it had been caught _in flagrante delicto_. In his belief, it
had no physical connection with, but was merely projected upon, the
nebula. But since then the nebular relations of blazing stars have
been strongly underlined. The mass of circumstantial evidence now
accumulated on the point fully warrants the assertion that Eta Argûs
makes an integral part of the formation it once illuminated.

A cluster in the constellation of the Cross, unique in the varied and
brilliant tints of its principal components, was compared by Herschel
to “a gorgeous piece of fancy jewellery.” Within the space of 1/48th
part of a square degree, he determined the places of no less than 110
of them, referred to Kappa Crucis, a rosy orb round which they are
irregularly scattered. The colour-effects in this beautiful ornament of
the sky need large apertures for their full display.

An object showing to the eye as a hazy star of the fourth magnitude
was entitled by Bayer in 1603 Omega Centauri. Herschel’s twenty-foot
disclosed it as “a noble globular cluster, beyond all comparison the
richest and largest in the heavens.” Dr. Gill obtained an admirable
photograph of it May 25, 1892. The stars composing it are literally
countless. On a plate exposed for two hours at Arequipa, Mr. Solon I.
Bailey reckoned nearly 6,400; yet he made no allowance for those “too
faint and closely packed” to be perceptible except as a “mottled grey
background between the distinct images.”

Somewhat inferior to Omega Centauri in size, though not at all in
beauty, is 47 Toucani. So obvious is it to the naked eye that, for
several nights after his arrival in Peru, Humboldt took it for a comet.
Central condensation in this cluster appeared to Herschel as if marked
off into three distinct stages; and to his delighted perception the
whole interior offered, by its roseate hue, an exquisite contrast to
the silvery radiance of the outer portions. No other observer has,
however, noticed this chromatic peculiarity. The structure of 47
Toucani is almost perfectly uniform. It is broken by none of the “dark
lanes,” rifts, or tunnels which so curiously diversify many globular
clusters. The usual hirsute aspect lent by the spreading abroad of
_tentacles_, or radiating stellar streams, is likewise scarcely
distinguishable either in 47 Toucani or Omega Centauri. Indeed, Mr.
Bailey noticed that the photographic images of both were all but
perfectly circular. In a future age this may be otherwise. Streams of
stars will, perhaps, set outward from these grand assemblages, leaving
vacancies behind. Thus, if it be permissible to judge of the relative
antiquity of clusters by their advance towards disruption, 47 Toucani
and Omega Centauri may be reckoned among the youngest of the globular
kind existing in the heavens.

The mechanism of clusters has received little attention from any
astronomer beside Herschel. And a solution of an ideal case of the
problem it presented was the utmost he could achieve.

“A quiescent spherical form,” he wrote in 1833, “may subsist as the
bounding outline of an immense number of equal stars, uniformly
distributed through its extent. In such a state of things each star
might describe an ellipse in any plane, and in any direction in that
plane, about the common centre without the possibility of collision.
If the form be not spherical, and the distribution of the stars not
homogeneous, the dynamical relations become too complicated to be
distinctly apprehended.”

But the more closely these aggregations are examined, the less likely
does it seem that they in any sense represent “quiescent forms.” The
arrangement of the stars composing them rather suggests their being
outward bound into the ocean of surrounding space, although the orders
that they carry are to us sealed.

Herschel subsequently altered his views regarding the composition
of clusters, and threw out in 1847 “the possibility of masses of
luminous matter--of whatever density or rarity, of whatever bulk or
minuteness--forming a connected system, and being prevented from
collapse or from mutual interference by the resistance of a transparent
and non-luminous medium.” For a “dynamical” he, in short, substituted
a “statical equilibrium,” the interposed medium lending unity to the
mixed aggregate, and enabling it to rotate, as a whole, upon an axis.
But the rotation is more than questionable. It seems to be precluded
by the ragged contours and indeterminate boundaries of all starry
collections. Photographic evidence, on the other hand, favours Sir John
Herschel’s surmise as to the composite nature of clusters. Some at
least evidently unite within themselves the “two sidereal principles.”
The stellar points they mainly consist of are immersed in, or linked
together by, shining nebulous stuff.

Herschel provided a southern sequel to his father’s star-gauging work
by counting 70,000 stars in 2,300 fields. Their distribution was in
complete accordance with the results of the earlier experiments.
“Nothing can be more striking,” Sir John wrote, “than the gradual,
but rapid increase of density on either side of the Milky Way as we
approach its course.” The existence of an “ecliptic of the stars” (in
Lambert’s almost prophetic phrase) was demonstrated. Or, as Herschel
himself put it, the plane of the Galaxy “is to sidereal, what the
ecliptic is to planetary astronomy, a plane of ultimate reference, the
ground-plan of the sidereal system.” He estimated, from the basis of
his gauge-reckonings, that his twenty-foot reflector was capable of
showing, in both hemispheres, about five and a half million stars. The
smallest of these would be of 14·5 magnitude, on the strict photometric
scale. But, unless his valuation was greatly too small, there must
be a conspicuous falling off in stellar density beyond the region of
tenth or eleventh magnitude. If this be so, scarcely one-quarter of
the expected stars will make their appearance on the plates of the
International Survey.

The grand feature of southern celestial scenery is the splendour of the
Milky Way. One of the galactic condensations in Sagittarius actually
seems to start out from the sky in a definite globular form; and the
darkness of the great rift beginning near the Cross is so intensified
by contrast with the strongly luminous branches it separates, as to
throw the blackness of the exterior heavens _into the shade_. This
part of the Milky Way may even be seen in southern latitudes--as it
was by the present writer--reflected from a glassy ocean-surface. The
section passing from Centaur through the Ship to Orion is, in some
respects, still more striking. Captain Jacob remarked at Madras that
“the general blaze from this portion of the sky is such as to render
a person immediately aware of its having risen above the horizon,
though he should not be at the time looking at the heavens.” Herschel
commented on the singular interruptions of the shining zone by obscure
spaces in Scorpio, near Alpha Centauri, and elsewhere; and admired
the enhancement afforded to its magnificence by “a marvellous fringe
of stars” attached pretty regularly to its southern border. “It is
impossible,” he wrote to Sir William Hamilton in June, 1836, “to resist
the conviction that the Milky Way is not a stratum, but a ring.”

His telescopic analysis disclosed in it a variety and complexity of
structure for which he was wholly unprepared. “Great cirrous masses
and streaks” of galactic light presented themselves in Sagittarius;
and, as the telescope moves, the appearance is that of clouds passing
in a _scud_.” “The Milky Way,” he continued, “is like sand, not strewn
evenly as with a sieve, but as if flung down by handfuls, and both
hands at once, leaving dark intervals, and all consisting of stars
of the lowest magnitudes,” down to nebulosity, in a most astonishing
manner.” As he proceeded, the stars became “inconceivably numerous and
minute. There must be millions on millions, and all most unequally
massed together; yet they nowhere run to nuclei, or clusters much
brighter in the middle.”

In some regions, the formation proved unfathomable; all traces of
stellar _texture_ disappeared. In others, it was plainly perceived to
consist of portions differing exceedingly in distance, but brought by
projection into nearly the same visual line. Near the Trifid Nebula,
“we see foreshortened,” he said, “a vast and illimitable area scattered
over with discontinuous masses and aggregates of stars, in the manner
of the cumuli of a mackerel-sky, rather than of a stratum of regular
thickness and homogeneous formation.”

These varied observations compelled him to reject decisively Olbers’s
hypothesis of light-extinction in space. For, if the possible range of
ethereal messages be restricted in one direction, it must be equally
restricted in all. “We are not at liberty,” he reasoned, “to argue that
in one part of the circumference of the galaxy our view is limited by
this sort of cosmical veil which extinguishes the smaller magnitudes,
cuts off the nebulous light of distant masses, and closes our view in
impenetrable darkness; while, at another, we are compelled, by the
clearest evidence telescopes can afford, to believe that star-strewn
spaces _lie open_, exhausting their powers and stretching out beyond
their utmost reach.” These objections seem fatal to what we may
call the “agnostic” theory of the sidereal world--the theory that
investigations into its construction are for ever barred by failure
of the means of communication--that we can never see more than a
necessarily meaningless part of a possibly infinite, and, in any case,
absolutely inscrutable whole.

The general telescopic exploration of the Milky Way began and ended
with the Herschels. Their great reflectors have been superseded by
the photographic camera. This particular application of its versatile
powers encountered special difficulties; but they were happily
overcome by Professor Barnard in July, 1889. A six-inch portrait
lens afforded the two chief requisites of a powerful light-grasp and
an extensive field; and plates exposed with it for some three hours
showed accordingly, for the first time, “in all their delicacy and
beauty” (to quote Professor Barnard’s words), “the vast and wonderful
cloud-forms, with their remarkable structure of lanes, holes, and black
gaps, and sprays of stars, as no eye or telescope can ever hope to see
them.” The work has since been continued by him and others, notably
by Mr. Russell at Sydney, and by Professor Max Wolf at Heidelberg,
so that the complete round of the “circling zone” will, before long,
have its varied aspects permanently recorded. They frequently present
strange and significant forms. Branching, leaf-like, spiral, elliptical
structures abound; individual stars are disposed in circlets, streams,
parallel rows, curves of sundry kinds. A “clustering power” of unknown
nature is ubiquitously active; orderly development is in progress.
A creative purpose can be _felt_, although it cannot be distinctly
followed by the mind.

Herschel’s “sweeps” in southern skies were continued until January,
1838; but with frequent intermissions. He was ready for every
interesting object that came in his way--comets among the rest.
“Encke’s--_yours_,” he informed his aunt, October 24, 1835, “escaped me
owing to trees and the Table Mountain, though I cut away a good gap in
our principal oak avenue to get at it.” Four days later he caught sight
of Halley’s comet at its second predicted return. But for the stellar
aspect of this body his observations of it would have begun much
earlier; for, in the absence of an exact ephemeris, it was impossible
to pick it out from among the stars it long precisely counterfeited.
“I am sure,” he said, “that I must often have swept with a night-glass
over the very spot where it stood in the mornings before sunrise; and
never was surprise greater than mine at seeing it riding high in the
sky, broadly visible to the naked eye, when pointed out to me by a note
from Mr. Maclear, who saw it with no less amazement on the 24th.”

“This comet,” he wrote to Miss Herschel, March 8, 1836, “has been a
great interruption to my sweeps, and I _hope_ and _fear_ it may yet
be visible another month.” It lingered on just two. He watched with
astonishment the changes it underwent. “Within the well-defined head,”
he wrote in his “Cape Observations,” “and somewhat eccentrically
placed, was seen a vividly luminous nucleus, or rather, an object
which I know no better way to describe than by calling it a miniature
comet, having a nucleus, head, and tail of its own, perfectly distinct,
and considerably exceeding in intensity of light the nebulous disc or
envelope.”

This strangely organised body was a very Proteus for instability of
form. It alternately lost and recovered its tail. It contracted into
the likeness of a star, then dilated into a nebulous globe, which
at last vanished as if through indefinite diffusion. The whole mass
“seemed touched, seemed turned to finest air.” During one week at
the end of January--it had passed perihelion November 16--Sir John
estimated that the cometary Amœba had increased its bulk no less than
forty times!

The paraboloidal form characteristic of this comet and many others, was
to him “inconceivable,” apart from the play of repulsive, in addition
to attractive forces; and he suggested that high electrical excitement
due to vaporisation, if of the same kind with a permanent charge on
the sun, would plausibly account for the enigmatical appearances he
had witnessed. From their close study at Königsberg, Bessel had
already concluded “the emission of the tail to be a purely electrical
phenomenon.”

In March, 1836, Herschel attacked the subject of southern stellar
photometry. Carrying further the “method of sequences,” he determined
the relative brightness of nearly five hundred stars, which he disposed
in order on a single descending scale, and linked on by careful
comparisons to the northern stars, as they “lightened into view” on the
homeward voyage. By the device of an “artificial standard star,” he was
besides enabled to obtain numerical values for the lustre of each star
examined, in terms of that of Alpha Centauri. Most important of all, he
rectified the current system of magnitudes, and introduced a definite
“light ratio,” which has since been extended, and more strictly
defined, but not altered.

His “astrometer” gave Herschel the means of _balancing_ the lustre of
Alpha Centauri against full moonlight. The latter proved to be 27,500
times more powerful. And Wollaston having determined the ratio of
moonlight to sunlight at 1/800000 (corrected by Zöllner to 1/600000),
it became feasible to compare the brightness of any particular star,
_as we see it_, with the brightness of the sun. Alpha Centauri, for
example, sends us, according to Herschel, 1/22 thousand millionth of
the light we receive from our domestic luminary. Moreover, when the
distance of the star came to be measured (it amounts to twenty-five
billions of miles), _light received_ could at once be translated into
_light emitted_. And the result has been to show that the components of
this splendid binary are, taken together, four times more luminous than
the sun. Through Sir John Herschel’s photometric researches, then, the
real light-power of stars at known distances became an ascertainable
quantity; and it is an element of great importance to astrophysical
inquiries.

On January 10, 1837, he wrote from Feldhausen to his brother-in-law:
“I am now at work on the spots in the sun, and the general subject
of solar radiation.” The sun was just then at an exceptionally high
maximum of disturbance. Spots of enormous size frequently obscured
its disc. One was estimated by Herschel, March 29, 1837, to cover,
independently of others, an area of 3,780 millions of square miles. So
that it considerably exceeded in dimensions the great spot-group of
February, 1892, the largest ever photographed at Greenwich. The study
of a series of such phenomena led him to propound the “cyclone-theory”
of their origin. It marked a decided advance in solar physics, if
only because it rested upon the fact--until then unaccountably
overlooked--that spot-production is intimately connected with the
sun’s rotation. He regarded it as a kind of disturbance incidental to
a system of fluid circulation analogous to the terrestrial trade- and
anti-trade winds. “The spots,” he said, “in this view of the subject
would come to be assimilated to those regions on the earth’s surface
where, for the moment, hurricanes and tornadoes prevail; the upper
stratum being temporarily carried downwards, displacing by its impetus
the two strata of luminous matter beneath, the upper of course to a
greater extent than the lower, and thus wholly or partially denuding
the opaque surface of the sun below.”

But the fundamental cause of our atmosphere’s flow and counter-flow
is absent in the sun. The earth is heated from the outside, and
therefore unequally; hence the air rushes along, turning westward
as it goes, from the chilly poles to the torrid zone of vertical
sunshine. No reason is, however, apparent why the solar equator should
be hotter than the solar poles. That adduced by Herschel is certainly
inadequate. He supposed that, by a retention of heat at the equator due
to the accumulation there, consequent upon his rotation, of the sun’s
absorbing atmosphere, a difference of temperature might be maintained
sufficient to keep the solar trade-winds blowing. But the effect is too
slight to be detected. And, in fact, the main drift of the photospheric
layers is along parallels of latitude. Polar and equatorial currents
are insignificant and uncertain.

Herschel and Pouillet contemporaneously, although at opposite sides
of the globe, succeeded in 1837 in measuring the intensity of solar
radiation. They were the first to apprehend the true bearings of the
question, which in principle are simple enough. All that is required
is to determine the heating effects, in a given time, of direct
sunshine. Its despoilment by our air has, indeed, to be allowed for.
Here the chief element of uncertainty comes in. Herschel put the loss
at one-third the original thermal power of vertical rays; Pouillet
pronounced it nearly one-half; Langley, using the most refined
appliances, concludes it to be four-tenths. Striking an average between
his own and the French results, Herschel calculated that, at the sun’s
surface, a shell of ice forty feet thick would melt in one minute, the
rate being reduced, at the distance of the earth, to an inch in two
hours and twelve minutes. And it is now practically certain that this
estimate was too small by about half its amount.

By way of illustrating the effects obtained with his philosophical
apparatus, he constructed a popular kind of actinometer, in the shape
of an “American dispatch,” made of a few pieces of wood and two panes
of glass, in which eggs were roasted, and beef-steaks broiled, by
sun-heat alone. The viands thus _cosmically cooked_ were “eaten with no
small relish by the entertained bystanders.”

Mimas and Enceladus, Saturn’s innermost moons, had persistently eluded
Herschel’s search for them in England; but, to his great delight, both
favoured him at the Cape. His observations of them in 1835–6 were the
first since his father’s time. The next detection of Mimas was by Mr.
Lassell in 1846.

The extent, variety, and completeness of the work done at Feldhausen
strike one with ever-fresh admiration. It seems scarcely credible that
so much was accomplished in four years by a single unaided individual.
Herschel’s only assistant was an honest mechanic named John Stone,
faithful, serviceable, in his way skilful, but not a “being” of the
“quick as lightning” sort, imagined and realised by Caroline Herschel.
It is related that during his observations of Halley’s comet, Sir John
on one occasion fell asleep, and while he remained in this condition
of peril (owing to the elevation and insecurity of his perch), Stone
kept dutifully turning the telescope. At last the astronomer awoke,
rubbed his eyes, looked down the great tube, saw nothing, rubbed his
eyes again, and exclaimed, “Why, John, where’s the comet?” The comet
had meantime set, and the telescope was duly directed towards its place
behind Table Mountain!

The splendid fulfilment of his astronomical tasks did not represent
the whole of Herschel’s activity at the Cape. He collected a large
store of tidal data for Dr. Whewell; started scientific meteorology;
established a system of national education still working beneficially,
and presided over the South African Literary and Scientific
Institution, the members of which presented him with a gold medal on
his departure. His visit made an epoch in the development of the Colony.

To himself personally it was a time of intense enjoyment. His labours,
arduous though they were, proceeded calmly, disembarrassed from
jostling claims and counter-claims. They were carried on with absorbed
enthusiasm, inspired in part by their sublime nature, in part by the
excitement of novelty. His family throve and multiplied at Feldhausen.
Sir Thomas Maclear’s friendship supplied unfailing social pleasure. An
exhilarating climate, moreover, enchanting scenery, translucent skies,
blossoming glens and hillsides worthy of Maeldune’s Isle of Flowers,
contributed to render his southern sojourn a radiant episode. He wrote
of it to Mr. Stewart as “the sunny spot in my whole life, where my
memory will always love to bask.” But “the dream,” he added, “was too
sweet not to be dashed by the dread of awakening.” The spell was broken
when in the middle of March, 1838, he sailed in the _Windsor Castle_
for England.

The interest created by his romantic expedition spread to the other
side of the Atlantic. A grotesque narrative, published in the _New
York Sun_ for September, 1835, of lunar discoveries made at the Cape
with the combined aid of the twenty-foot reflector and the Drummond
limelight, was eagerly read and believed by thousands, was reprinted,
re-circulated, and re-read. Nor were common gulls the only victims
to the hoax. The truth of the story was gravely debated by the Paris
Academy of Sciences.

Herschel’s home-coming was a triumph. He was overwhelmed with applause
and gratulation. His fellow-countrymen offered him what compensation
they could for the disappearance from his horizon of the Southern
Cross. He was created a baronet at the Queen’s Coronation, received
an honorary degree of D.C.L. at Oxford in 1839, and was offered, but
declined, reimbursement from the Treasury for the entire cost of his
trip. He peremptorily refused as well to represent the University of
Cambridge in Parliament, or to be nominated for the Presidentship of
the Royal Society. His utmost desire was for a quiet and laborious
life. A banquet, however, given in honour of his return, June 15,
1838, could not be shunned; the less so that the celebration had a
typical character. “In honouring a man,” Sir William Hamilton said, in
proposing his health, “we honour science too.” For “the cultivators and
lovers of Science have chosen Herschel for their chief--say, rather,
have as such received him by inheritance.”




CHAPTER IX.

LIFE AT COLLINGWOOD.


Herschel’s career as an observing astronomer came to a virtual end with
his departure from the Cape. He was then forty-six, two years younger
than his father when he began his course of prodigious activity at
Slough. Sir William’s craving to see and to know was insatiable; Sir
John’s was appeased by the accomplishment of one grand enterprise. His
was a many-sided mind; dormant interests of sundry kinds revived on the
first opportunity; new ones sprang up; and curiosity to interrogate the
skies ceased to “prick the sides of his intent.” So the instruments
taken down at Feldhausen in 1838 were not remounted in England; and
their owner is never again recorded to have used a telescope. One
cannot but regret that, in the plenitude of his powers, and instructed
by rare experience, he should have put by his weapons of discovery.[H]
The immense stock of observations with which they had furnished him
remained, it is true, in their primitive, rough-hewn state; and he may
have considered that wise husbandry required him to save one harvest
before planting another. This, at any rate, was the course that he
pursued.

    [H] The three specula of the twenty-foot are in the possession
        of Sir William J. Herschel; the tube remains in good
        preservation at Collingwood.

But it was often and in many ways interrupted. The demands on his
time and thoughts were innumerable. Having settled his family
for the season in London, he paid his third and last visit to his
venerable aunt, and, in returning, dined with Dr. Olbers, the
physician-astronomer of Bremen, then in his eightieth year. A fortnight
later he was on his way to Newcastle, where the British Association
met, August 20th. He was received with acclamation, but overwhelmed
by scientific exactions. The proceedings were to him “a dreadful wear
and tear,” and they left behind “mixed and crowded recollections.” No
wonder. Besides acting as President of the Mathematical Section, he
found himself involved in varied responsibilities. He was placed on a
Committee for bringing down to date the places of Lacaille’s 10,000
southern stars; on another for revising stellar nomenclature. The
reduction of a body of meteorological observations made on a plan of
his devising was entrusted to him; above all, he was charged with the
development of Humboldt’s international scheme for securing systematic
and world-wide observations on terrestrial magnetism. He drew up a
memorial to the Government; compiled the Instructions for Sir James
Clark Ross’s Antarctic expedition; and elaborately reported progress
at several successive meetings of the British Association. His heart
was in the work. He contributed an article dwelling on its importance
to the _Quarterly Review_ for June, 1840; and in 1845 he expressed the
opinion that “terrestrial physics form a subject every way worthy to be
associated with astronomy as a matter of universal interest and public
support.”

The constellations gave him still more trouble than the vagaries of
poised needles. They were in a riot of disorder. Celestial maps had
become “a system of derangement and confusion”--of confusion “worse
confounded.” New asterisms carved out of old existed precariously,
recognised by some, ignored by others; waste places in the sky had
been annexed by encroaching astronomers as standing-ground for their
glorified telescopes, quadrants, sextants, clocks; a chemical apparatus
had been set up by the shore of the river Eridanus, itself a meandering
and uncomfortable figure; while serpents and dragons trailed their
perplexing convolutions through hour after hour of right ascension.
There were constellations so large that Greek, Roman, and Italic
alphabets had been used up in designating the included stars; there
were others separated by debatable districts, the stars in which often
duplicated those situated within the authentic form of one of the
neighbouring celestial monsters. Identification was thus in numberless
cases difficult; in some, impossible.

In conjunction with Francis Baily, Herschel undertook the almost
hopeless task of rectifying this intolerable disorder. After much
preliminary labour, he submitted to the Royal Astronomical Society,
in 1841, a drastic scheme of constellational reform--a stellar
redistribution-bill, framed on radical principles. Its alarming
completeness, however, caused it to be let drop; and he finally
proposed, in his report of 1844 to the British Association, a less
ambitious but more practicable measure. Although not adopted in its
entirety, it paved the way for ameliorations. The boundaries of
the constellations have since been defined; interlopers have been
ejected; one--the Ship Argo--especially obnoxious for its unwieldy
dimensions, has been advantageously trisected. Nevertheless, individual
star-nomenclature grows continually more perplexed; partial systems
have become intermingled and entangled; double stars are designated in
one way, variables in another, quick-moving stars in a third, red stars
in a fourth, while any one of many catalogue-numbers may be substituted
at choice; palpable blunders, unsettled discrepancies, anomalies of
all imaginable kinds, survive in an inextricable web of arbitrary
appellations, until it has come to pass that a star has often as many
aliases as an accomplished swindler.

In the spring of 1840 Herschel removed from Slough to Collingwood,
a spacious country residence situated near Hawkhurst, in Kent. Here
he devoted himself, in good earnest, to the preparation of his Cape
results for the press. It was no light task. The transformation of
simple registers of sweeps into a methodical catalogue is a long and
irksome process; and Herschel was in possession of the “sweepings”
of nearly four hundred nights. He executed it single-handed, being
averse to the employment of paid computers. This was unfortunate.
Monotonous drudgery was not at all in his line; as well put Pegasus
between shafts. He had always found in himself “a great inaptitude”
for numerical calculations; and he now acknowledged to Baily that
attention to figures during two or three consecutive hours distressed
him painfully. Whewell lamented in the _Quarterly Review_ the lavish
expenditure of his time and energy upon “mere arithmetic”--computations
which a machine would have been more competent to perform than a
finely organised human brain. At last, however, in November, 1842, the
necessary reductions were finished; and the letterpress to accompany
the catalogues of double stars and nebulæ left his hands a couple of
years later. The preparation of the plates occasioned further vexatious
delays; and it was not until 1847 that the monumental work entitled
“Results of Astronomical Observations at the Cape of Good Hope” issued
from the press. The expenses of its production were generously defrayed
by the Duke of Northumberland. In sending a copy to his aunt, then in
her ninety-eighth year, he wrote: “You will have in your hands the
completion of my father’s work--‘The Survey of the Nebulous Heavens.’”
The publication was honoured with the Copley Medal by the Royal
Society, and with a special testimonial by the Astronomical Society.

Bessel, the eminent director of the Königsberg observatory, made
Herschel’s personal acquaintance at the Manchester meeting of the
British Association in 1842, and paid him a visit at Collingwood. The
subject of a possible trans-Uranian planet was discussed between them.
The German astronomer regarded its existence as certain, and disclosed
the plot he had already formed for waylaying it on its remote path. The
premonition stirred Herschel deeply. “There ought to be a hue and cry
raised!” he exclaimed in a letter to Baily. And in resigning the Chair
of the British Association, September 10, 1846, he spoke with full
assurance of the still undiscovered body. “We see it,” he declared,
“as Columbus saw America from the shores of Spain. Its movements have
been felt, trembling along the far-reaching line of our analysis, with
a certainty hardly inferior to that of ocular demonstration.” Within a
fortnight, Neptune, through Le Verrier’s indications, was captured at
Berlin.

“I hope you agreed with me,” he wrote, November 19, 1846, to Sir
William Hamilton, “that it is perfectly possible to do justice to
Adams’s investigations without calling in question M. Le Verrier’s
_property_ in his discovery. The fact is, I apprehend, that the
Frenchmen are only just beginning to be aware _what a narrow escape Mr.
Neptune had of being born an Englishman_. Poor Adams aimed at his bird,
it appears, first, and as well as Le Verrier, but his gun hung fire,
and the bird dropped on the other side of the fence!”

It is well known that Le Verrier and Adams personally ignored
controversy as to their respective claims to the planetary _spolia
opima_. They were together at Collingwood in July, 1847, with Struve as
their fellow-guest. During those few days King Arthur (in the person of
Sir John Herschel) “sat in hall at old Caerleon.”

He was elected President of the Royal Astronomical Society for the
usual biennial term in 1828, 1840, and 1847; on the last occasion
through the diplomatic action of Professor De Morgan. The Society
was passing through a crisis; he apprehended its dissolution, and
judged that it could only be saved by getting Herschel’s consent to
become its nominal head. “The President,” he wrote to Captain Smyth,
“must be a man of brass (practical astronomer)--a micrometer-monger,
a telescope-twiddler, a star-stringer, a planet-poker, and a
nebula-nabber. If we give bail that we won’t let him do anything if he
would, we shall be able to have him, I hope. We must all give what is
most wanted, and his name is even more wanted than his services. We can
do without his services, not without loss, but without difficulty. I
see we shall not, without great difficulty, dispense with his name.”

And to Herschel himself: “We have been making our arrangements for
the Society for the ensuing year; and one thing is that you are not
to be asked to do anything, or wished to do anything, or wanted to do
anything. But we want your _name_.” It was lent; and its credit seems
to have had the desired effect.

Dr. Whewell vainly tried to inveigle him, in November, 1838, into
accepting the presidentship of the Geological Society; but he had to
submit, in 1842, to be elected Rector of Marischal College, Aberdeen;
and he consented to preside over the meeting of the British Association
at Cambridge in June, 1845. His dignity on the occasion was not allowed
to interfere with his usefulness. He wrote home June 22: “We have been
on the Magnetic Committee working hard all the morning, in a Babel of
languages and a Babylonian confusion of ideas, which crystallised into
something like distinctness at last.” By that time the long-desired
particulars regarding terrestrial magnetism were rapidly accumulating.
_Facts_, as Herschel announced from the Presidential Chair, were
plentifully at hand. “What we now want is _thought_, steadily directed
to single objects, with a determination to avoid the besetting evil
of our age--the temptation to squander and dilute it upon a thousand
different lines of inquiry.”

Herschel observed the great comet of 1843 from the roof of his house
at Collingwood, on March 17, the first evening of its visibility in
England. All that could be seen was “a perfectly straight narrow band
of considerably bright, white cloud, thirty degrees in length, and
about one and a half in breadth.” It was not until the following night
that he recognised in this strange “luminous appearance” “the tail of
a magnificent comet, whose head at the times of both observations was
below the horizon.”

In December, 1850, he was appointed Master of the Mint--a position
rendered especially appropriate to him by Newton’s prior occupation of
it. The duties connected with it were just then peculiarly onerous.
Previously of a temporary and political character, the office now
became permanent, and simply administrative. Many other changes
accompanied this fundamental one. “The whole concern,” he said, “is in
process of reorganisation.” This fresh start demanded much “personal
and anxious attendance.” Notwithstanding his anxious regard for the
interests of subordinates, the reconstruction could not but be attended
by serious friction. No amount of oiling will get rusty wheels to
revolve smoothly all at once. “Things progress rather _grumpily_,” he
reported privately, “owing to the extreme discontent of some parties.”
Further contentious business devolved upon him as a member of the
jury on scientific instruments at the Great Exhibition. His time was
fully and not agreeably occupied. Rising at six, he worked at home
until half-past nine, then hurried to the Mint, which he exchanged
between three and four o’clock for the Exhibition, and there, until the
closing of its doors, examined the claims, and appeased the quarrels of
rival candidates for distinction. He also sat on the Royal Commission
appointed in 1850 to inquire into the University system. Its
recommendations, agreed to by him in 1855, greatly disgusted Whewell;
but their friendship remained unaltered by this discordance of opinion.

These accumulated responsibilities were too much for Herschel’s
sensitive nature; and the burthen was made heavier by a partial
separation from his family. He was never alone in Harley Street, but
the joyous life of Collingwood could not be transported thither;
and the arid aspect of a vast metropolis, suggesting business and
pleasure in excess, but little of enjoyment in either, oppressed him
continually. His health suffered, and in 1855 he withdrew definitively
into private life. His resignation of the Mint was most reluctantly
accepted.

“I find,” playfully remarked De Morgan, “that Newton and Herschel added
each one coin to the list: Newton, the gold quarter-guinea, which was
in circulation until towards the end of the century; Herschel, the gold
quarter-sovereign, which was never circulated.”

It was not the repose of inaction that Herschel sought at Collingwood.
“Every day of his long and happy life,” Professor Tait said truly,
“added its share to his scientific services.” Thenceforward he devoted
himself chiefly to the formidable task of collecting and revising
his father’s results and his own. His “General Catalogue of Nebulæ,”
published in the _Philosophical Transactions_ for 1864, was in itself
a vast undertaking. It comprised 5,079 nebulæ and clusters, to which
it served as a universal index of reference. It averted the mischief
of duplicate discoveries, settled the sidereal status of many a
pseudo-comet, and quickly became the authoritative guide of both
comet- and nebula-hunters. In the enlarged form given to it by Dr.
Dreyer in 1888, it is likely long to hold its place. Herschel next, in
1867, amalgamated into a regular catalogue of 812 entries his father’s
various classed lists of double stars (Memoirs, Royal Astronomical
Society, xxxv.). A far more comprehensive work was then taken in hand.
He desired to do for double stars what he had done for nebulæ--to
compile an exhaustive register of them in the shape of a catalogue,
accompanied by a short descriptive account of each pair. But he was not
destined to put this coping-stone to the noble monument erected by his
genius. Strength failed him to digest and dispose the immense mass of
materials he had collected. Nor was it possible for another to gather
up the loose threads of his unfinished scheme. All that could be done
was to preserve the imposing fragment as he left it. An ordered list
of the 10,320 multiple stars he had proposed to treat was accordingly
published in the fortieth volume of the same Society’s _Memoirs_ under
the care of Professor Pritchard and Mr. Main. But it hardly possesses
more than a commemorative value.

Maria Edgeworth was an old friend of Sir John Herschel’s. In March,
1831, she paid him a three days’ visit at Slough, which, she told a
friend in Ireland, “has far surpassed my expectations, raised as they
were, and warm from the fresh enthusiasm kindled by his last work” (the
“Preliminary Discourse”). Mrs. Herschel she described as “very pretty,”
sensible, and sympathetic, and possessed of the art of making guests
happy without effort. On Sunday, after service, the philosopher showed
off the dazzling colour-effects of polarised light, and at night,
with the twenty-foot, “Saturn and his rings, and the moon and her
volcanoes.”

After twelve years, she came again, this time to Collingwood. “I should
have written before,” Herschel assured Sir William Hamilton, December
1st, 1843, “but Miss Edgeworth has been here, and that, among all
people who know how to enjoy her, is always considered an excellent
reason for letting correspondence and all other worldly things ‘gang
their ain gate.’ She is more truly admirable now, I think, than at any
former time, though in her seventy-fifth year.”

Maria herself wrote from Collingwood in the following spring: “Here are
Lord and Lady Adare, Sir Edward Ryan, and ‘Jones on Rent.’ Jones and
Herschel are very fond of one another, always differing, but always
agreeing to differ, like Malthus and Ricardo.”

Sir William Hamilton spent a week under the same hospitable roof in
1846. He was delighted, and, as was his wont, compressed the expression
of his pleasure “within the Sonnet’s scanty plot of ground.” In the
first of a pair entitled “Recollections of Collingwood,” he celebrated
the “thoughtful walk” with his host, and the “social hours” in a family
circle,

     “Where all things graceful in succession come;
      Bright blossoms growing on a lofty stalk,
      Music and fairy-lore in Herschel’s home.”[I]

    [I] The lines are quoted in Graves’s “Life of Hamilton,” vol.
        ii. p. 525.

The second dealt with “high Mathesis,” and

              “dimly traced Pythagorean lore;
      A westward-floating, mystic dream of FOUR.”

Although not, like his friend, an incorrigible and impenitent
sonnetteer, Herschel was “very guilty” of at least one specimen of the
art. They were staying together, in June, 1845, at Ely, in the house of
Dean Peacock. Hamilton’s inevitable sonnet came duly forth, and “next
morning,” he related to De Morgan, “as my bedroom adjoined Herschel’s,
and thin partitions did my madness from his great wit divide, I easily
heard what Burns might have called a ‘crooning,’ and was not much
surprised (being familiar with the symptoms of the attack)[J] when,
before we sat down to breakfast at the Deanery, Lady Herschel handed
me, in her husband’s name and her own, a sonnet of _his_ to _me_,
which, unless the spirit of egotism shall seize me with unexpected
strength, I have no notion of letting you see.”

    [J] “Aut insanit, aut versos facit.”

The circulation of Herschel’s fervid eulogy would assuredly have put
his modesty to the blush. Headed “On a Scene in Ely Cathedral,” it runs
as follows:--

     “The organ’s swell was hushed, but soft and low
      An echo, more than music, rang; when he,
      The doubly-gifted, poured forth whisperingly,
      High-wrought and rich, his heart’s exuberant flow
      Beneath that vast and vaulted canopy.
      Plunging anon into the fathomless sea
      Of thought, he dived where rarer treasures grow,
      Gems of an unsunned warmth and deeper glow.
      O born for either sphere! whose soul can thrill
      With all that Poesy has soft or bright,
      Or wield the sceptre of the sage at will
      (That mighty mace which bursts its way to light),
      Soar as thou wilt!--or plunge--thy ardent mind
      Darts on--but cannot leave our love behind.”

Of Hamilton’s abstruse invention, the method of “Quaternions” (here
alluded to), Herschel was, from the first, an enthusiastic admirer.
He characterised it in 1847 as “a perfect cornucopia, from which, turn
it on which side you will, something rich and valuable is sure to drop
out.” The “power and pregnancy” of the new calculus were supremely
delightful to him, and he advised every mathematician to gain mastery
over it as a “working tool.” As such it has not yet been brought into
ordinary use, yet it remains in the armoury of science, ready for
emergencies.

Miss Mitchell of Nantucket, the discoverer of a comet, and a professor
of astronomy, published in 1889 (in the _Century_ magazine) her
reminiscences of a short stay at Collingwood in 1858. Her host “was
at that time sixty-six, but he looked much older, being lame and much
bent in his figure. His mind, nevertheless, was full of vigour. He
was engaged in re-writing the ‘Outlines of Astronomy.’” “Sir John’s
forehead,” she says, “was bold but retreating; his mouth was very good.
He was quick in motion and in speech. He was remarkably a gentleman;
more like a woman in the instinctive perception of the wants and wishes
of a guest.”

“In the evening,” she relates, “we played with letters, putting out
charades and riddles, and telling anecdotes, Sir John joining the
family party and chatting away like the young people.” He propounded
the question: If one human pair, living in the time of Cheops, had
doubled, and their descendants likewise, once every thirty years, could
the resulting population find room on the earth? The company thought
not. “But if they stood closely, and others stood on their shoulders,
man, woman, and child, how many layers would there be?” “Perhaps
three,” replied Miss Mitchell. “How many feet of men?” he insisted.
“Possibly thirty.” “Enough to reach to the moon,” said his daughter.
“To the sun,” exclaimed another. “More, more!” cried Sir John, exulting
in the general astonishment. “To Neptune,” was the next bid. “Now you
burn,” he allowed. “_Take one hundred times the distance of Neptune,
and it is very near._” “That,” he added, “is my way of whitewashing
war, pestilence, and famine.”

He further entertained his American guest with accounts of the
paradoxical notions communicated to him by self-taught or would-be
astronomers. One had inferred the non-existence of the moon from
Herschel’s chapters on lunar physics and motions. Another enclosed
half-a-crown for a horoscope. A third wrote, “Shall I marry, and have
I seen her?” In reference to the efforts then being made to introduce
decimal coinage into England, he remarked, “We stick to old ways, but
we are not cemented to them.”

The portrait of Caroline Herschel, painted by Tielemann in 1829,
which she herself declared to “look like life itself,” hung in the
drawing-room. (It is that reproduced in this volume.) “You would say in
looking at it,” Miss Mitchell wrote, ‘she must have been handsome when
she was young.’ Her ruffled cap shades a mild face, whose blue eyes
were even then full of animation. But it was merely the beauty of age.”

Herschel was no exception to the rule that astronomers love music
and flowers. He was never tired of gardening, and--to quote James
Nasmyth--“his mechanical and manipulative faculty enabled him to take a
keen interest in all the technical arts which so materially aid in the
progress of science.” The manufacture of specula naturally came home
to him, and he watched with genuine pleasure Nasmyth’s grinding and
polishing operations. He spent several days with him at Hammerfield in
1864. “Of all the scientific men I have had the happiness of meeting,”
Nasmyth wrote in his “Autobiography,” “Sir John stands supremely at
the head of the list. He combined profound knowledge with perfect
humility. He was simple, earnest, and companionable. He was entirely
free from assumptions of superiority, and, still learning, would listen
attentively to the humblest student. He was ready to counsel and
instruct, as well as to receive information.”

Herschel’s correspondence with De Morgan extended over nearly forty
years, and became latterly of an intimate character. “Looking back on
our long friendship,” he wrote to the widow shortly after De Morgan’s
death in the spring of 1871, “I do not find a single point on which we
failed to sympathise; and I recall many occasions on which his sound
judgment and excellent feeling have sustained and encouraged me. Many
and very distinct indications tell me that I shall not be long after
him.”

It fell out as he had predicted. The obituary memoirs of the two are
printed close together in the Astronomical Society’s “Monthly Notices.”
After a prolonged decline of strength, Sir John Herschel died at
Collingwood, in his seventy-ninth year, May 5th, 1871, his intellect
remaining unclouded to the last. He was buried in Westminster Abbey,
near the grave of Newton. The words engraven above his resting-place,
“Coelis exploratis, hic prope Newtonum requiescit,” tell what he did,
and what he deserved.

His death created an universal sense of sorrow and of loss. He left
vacant a place which could never be filled. His powers, his qualities,
and his opportunities made a combination impossible to be reproduced.
His genius showed curious diversities from his father’s. He lacked
his profound absorption, his penetrating insight, his unaccountable
intuitions. A tendency to discursiveness, happily kept in check
by strength of will and devotion to an elevated purpose, replaced
in him his father’s enraptured concentration. On the other hand,
his appreciative instinct for the recondite beauty of mathematical
conceptions was wanting to his father. William Herschel possessed fine
mathematical abilities; but he cultivated them no further than was
necessary for the execution of his designs; and elementary geometry
served his turn. But Sir John might have taken primary rank as a pure
mathematician. Possibly his inventive faculty would have developed
in that line more strongly than in any other. The grasp of his mind
was indeed so wide that many possibilities of greatness were open
to him. That he chose rightly the one to make effective, no one
can doubt. The neglect on his part of astronomy would have been a
scientific delinquency. His splendid patrimony of telescopic results
and facilities was inalienable. It was a talent entrusted to him,
which he had not the right to bury in the ground. He laboured with it
instead to the last farthing. Not for his own glory. He aspired only
to fill up, for the honour of his father’s name, the large measure of
his achievements. In doing so he performed an unparalleled feat. He
swept from pole to pole the entire surface of the hollow sphere of the
sky. It is unlikely to be repeated. The days of celestial pioneering
are past. Nothing on the scale of a general survey will in future
be undertaken except with photographic help. The use of the direct
telescopic method tends to become more and more restricted. This is
a loss as well as a gain. A _hortus siccus_ is to a blooming garden
very much what a collection of photographs is to the luminous flowers
of the sky. They are depicted more completely, more significantly,
more conveniently for purposes of investigation, than they can be
seen; but the splendour of them is gone. Their direct contemplation
has an elevating effect upon the mind, which indirect study, however
diligent and instructive, is incapable of producing. The sublimity of
the visions drawn from the abyss of space cannot be reasoned about. It
strikes home to the spectator’s inner consciousness without waiting for
the approval of his understanding. Thus to Herschel, no less expressly
than to the Psalmist three thousand years earlier, “the heavens told
the glory of God.” He lived at his telescope a life apart, full of
incommunicable experiences.

“To Herschel,” as Mr. Proctor expressed it, “astronomy was not a
matter of right ascension and declination; of poising, clamping, and
reading-off; of cataloguing and correcting.” “It was his peculiar
privilege,” Dean Stanley remarked in his funeral sermon, “to combine
with those more special studies such a width of view and such a power
of expression as to make him an interpreter, a poet of science, even
beyond his immediate sphere.” Hence the popularity of his books, and
the favoured place he occupied in public esteem.

His character was of a more delicate fibre than his father’s. It was
also, by necessary consequence, less robust. Sir William Herschel
surmounted adversity. Sir John would have endured it, had his lot been
so appointed. But it never came his way. He was one of those rarest of
rare individuals--

     “Whose even thread the Fates spin round and full,
      Out of their choicest and their whitest wool.”

His life was a tissue of felicities. For him there was no weary
waiting, no heart-sickening disappointment, no vicissitudes of
fortune, no mental or moral tempests. Success attended each one of
his efforts; he could look back without regret; he could look forward
with confident hope; his family relations brought him unalloyed
happiness. He suffered, indeed, one bereavement in the untimely death
of his daughter, Mrs. Marshall, the wife of a nephew of Dr. Whewell;
but Christian resignation sweetened his sorrow. His religion was
unpretending and efficacious. No duty was left by him unfulfilled; and
he wore, from youth to age, “the white flower of a blameless life.”
A discriminating onlooker said of him, that his existence “was full
of the serenity of the sage and the docile innocence of a child.”
He was retiring almost to a fault, careless of applause, candid
in accepting criticism. Although habitually indulgent, he was no
flatterer, “Anyone,” Mr. Proctor said, “who objected to be set right
when in error, might well be disposed to regard Sir John Herschel as
a merciless correspondent, notwithstanding the calm courtesy of his
remarks. He set truth in the first place, and by comparison with her,
neither his own opinions, nor those of others, were permitted to have
any weight whatever.” Beginners invariably met with his sympathy and
encouragement. He felt for difficulties which he himself had never
experienced.

Being thus constituted, he could not but inspire affection. The French
physicist, Biot, when asked by Dr. Pritchard, after the death of
Laplace, who, in his opinion, was his worthiest successor, replied,
“If I did not love him so much, I should unhesitatingly say, John
Herschel.” His own attachments were warm and constant; and the few
scientific controversies in which he engaged, were carried on with his
habitual gentleness and urbanity.

Herschel left eight daughters and three sons, of whom the eldest, Sir
William James Herschel, succeeded him in the baronetcy, while the
second, Professor Alexander Stewart Herschel, has earned celebrity
by his meteoric researches. The election of the third, Colonel John
Herschel, to a Fellowship of the Royal Society, in recognition of his
spectroscopic examination of southern nebulæ, threw a gleam of joy over
his father’s deathbed. Lady Herschel survived her husband upwards of
thirteen years.

The learned societies of Europe vied with each other in enrolling
the name of Sir John Herschel; and he was nominated, in 1855, on the
death of Gauss, one of the eight foreign members of the French Academy
of Science. As we have seen, he received the Copley Medal from the
Royal Society twice, their Royal Medal thrice, and from the Royal
Astronomical Society, two Gold Medals and a testimonial. Compliments
and homage, however, left him as they found him--quiet, intent, and
unobtrusive.

Several portraits of him are in existence. One was executed in oils
by Pickersgill for St. John’s College, Cambridge, at a comparatively
early period of his life. It is here (page 142) reproduced from an
admirable engraving. His later aspect is finely represented in a
painting by his eldest daughter, Lady Gordon. The eyes in it are
sunken, though brilliant; the shape of the head is concealed by a
mane of grey hair. There is about it something of leonine grandeur,
disjointed from leonine fierceness. It perpetuates, indeed, the
countenance of a man replete with human tenderness.




CHAPTER X.

WRITINGS AND EXPERIMENTAL INVESTIGATIONS.


Could the whole of Sir John Herschel’s astronomical career be
obliterated, and the whole of his contributions to pure mathematics be
forgotten, he would still merit celebrity as a physicist. Experimental
optics, above all, engaged his attention. “Light,” he himself said,
“was his first love,” and he was never wholly forgetful of it. In 1830
he described himself as “forcibly drawn aside from his optical studies”
by the claims of nebulæ and double stars. How strong he felt those
claims to be, can best be understood by considering the firmness with
which he averted his mind, out of regard to them, from the intricate
and bewitching subject of his early devotion.

“I understand from Peacock,” Dr. Whewell wrote to him, June 19, 1818,
“that you are untwisting light like whipcord, examining every ray that
passes within half a mile, and putting the awful question, ‘Polarised,
or not polarised?’ to thousands that were never before suspected of any
intention but that of moving in a straight line.” These interrogatories
brought out a remarkable diversity in the action upon light of quartz,
and other similar substances, corresponding with the two different
modes of crystallisation belonging to each of them. Here, in Lord
Kelvin’s phrase, is “one of the most notable meeting-places between
natural history and natural philosophy.”

The nascent science of spectrum analysis was materially promoted by
Herschel. He noticed in 1819 the distinctive light-absorbing qualities
of coloured media, studied the spectra of various flames, adverted
to the definiteness and individuality of the bright lines composing
them, and recommended their employment for purposes of chemical
identification.

A year later, he developed and modified Brewster’s explanation of the
colours of mother-of-pearl. They do not, like the iridescence of a
fly’s wing, result from the interference of waves of light reflected
from two closely adjacent surfaces, but from interference brought about
by the finely striated texture of the shell’s surface, and a cast of
the rainbow-tinted surface in black sealing-wax will display the same
sheen of colour as the original. Herschel detected, however, a second
more closely striated structure which cannot be impressed upon plastic
matter.

Up to this time he accepted unreservedly the emission theory of
light. But a candid study of Young’s and Fresnel’s writings produced
a fundamental change in his opinions; and in an article on “Light,”
written for the “Encyclopædia Metropolitana” in 1827, he expounded
the undulatory theory with all the ardour of a neophyte. He brought
thereby one of the grandest generalisations of science into universal
currency, and enforced its acceptance by the cogency of his
arguments, the logical order of his method, and the lucidity of his
style. The treatise was translated into French by Quetelet; and no
reader, Professor Pritchard remarked, “could escape the charm of the
half-suppressed enthusiasm which carried him along.”

Whewell ranked him “among the _very_ small number of those who, in the
singularly splendid and striking researches of physical optics, had
both added important experimental laws to those previously known, and
weighed the relations of these discoveries to the refined and recondite
theory towards which they seemed to point.” He contributed to the
same Encyclopædia scarcely less brilliant essays on Heat, Sound, and
Physical Astronomy.

“Do not observe too much in cold weather,” Miss Herschel advised her
nephew, in anticipation of the winter of 1831–2; “write rather books to
make folks stare at your profound knowledge.”

He followed the positive part of her counsel. Indeed, his “Preliminary
Discourse on the Study of Natural Philosophy” had made its appearance
in the previous year, as the introductory volume to Lardner’s “Cabinet
Cyclopædia.” It was greeted with a chorus of approbation. Gauss
reviewed it in the _Gelehrte Anzeigen_, Whewell in the _Quarterly
Review_. Translated into French, German, and Italian, it delighted
“all sorts and conditions” of readers with the justice and breadth of
the views set forth in it agreeably, easily, and without pretension
to superiority. The book included a survey of the actual state
of scientific knowledge, and a philosophy of its augmentation.
Students derived from it, Gauss remarked, both information as to how
accepted results had been obtained, and guidance for their personal
investigations. Herschel was exceptionally qualified, Whewell wrote,
“to expound the rules and doctrines of that method of research to which
modern science has owed its long-continued, steady advance, and present
flourishing condition.” He had the knowledge, without the narrowness,
of a specialist in almost every department of experimental physics.
“With singular alacrity,” he came to the front wherever there seemed a
chance of pushing back the barriers of ignorance. A disciple of Bacon,
he had the advantage over his master of being habitually conversant
with the practical working of inductive methods. The treatise was
styled by Whewell “an admirable comment on the ‘Novum Organum.’” One,
however, possesses the indefinable quality of _greatness_; it stands
out from the centuries a solid structure, clothed with visionary
magnificence; the other is elegant, attractive, wise, acute, even
profound, but not in any degree, or from any point of view, _great_.

It was followed, in 1833, by “A Treatise on Astronomy,” published in
the same series. An “Edinburgh Reviewer” (doubtless Brougham once more)
perused it with regret. “The proper position of Sir John Herschel” he
considered to be “at the head of those who are nobly, though it may
be silently and without notice, endeavouring to extend the present
limits of human knowledge,” rather than among “the ranks of those whose
office it is to herald the triumphs of science, and point out its
treasures and results to the admiration of the vulgar.” This ostensibly
flattering estimate was made the basis for an imputation of vanity. The
inducements, according to the critic, were strong “to descend from the
airy summits of abstract science to the level at which the great body
of the reading public can appreciate and applaud. Philosophers, like
other writers, naturally wish to be read, and to have reputation; and
reputation, as was remarked by d’Alembert, depends more upon the number
than the merit of those who praise.” Sir John Herschel would have been
better employed in pursuing the track of original discoveries, leaving
new truths to “find their way to the drawing-room as best they might.”
The whole tenour of his life refuted these insinuations.

The “Treatise on Astronomy” was enlarged in 1849 into the deservedly
famous “Outlines of Astronomy.” Twelve editions of this book were
published, the last in 1873; it was translated into Chinese and Arabic,
as well as into most European languages, including Russian; it made a
profound and lasting impression upon the public mind. No science has
perhaps ever received so masterly a general interpretation. Methodical
in plan, inspiriting in execution, it demands readers willing to share
some part of the pains, for the sake of partaking in the high pleasures
of the writer. For it is popular in the sense of eschewing mathematical
formulæ, not in the sense of evading difficulties.

The work fittest to be set by its side is the “Exposition du Système
du Monde.” But Laplace restricted his view to the sun’s domain, while
Herschel excluded from his no part of the sidereal universe. Laplace
was, besides, a geometer in the first, an astronomer only in the second
place. The movements of the heavenly bodies interested him because
they afforded opportunities for analytical triumphs. Their intricacy
notwithstanding, he was elated to find that they could not baffle his
ingenuity in constructing formulæ to correspond. Their balance, their
harmony, their obedience to a single and simple law, gratified the
orderly instincts of his powerful yet frigid mind. Where he could not
explain, however, he did not admire. Mystery had no attraction for
him. Knowledge, to _be_ knowledge in his eyes, should have definite,
clear-cut outlines. His scheme of the universe was like the map of the
world laid down by Hecatæus, neatly finished off with a circumfluent
ocean-stream; it included no intimations of a _beyond_. Herschel’s, on
the contrary, might be compared to the map of Herodotus, in which some
details were filled in, while the external boundary had been abolished.
The most essential part of the progress made in the interval consisted
in leaving verge and scope for the unknown. Next to nothing remained
to be learned of the heavens, as they presented themselves to the
author of the “Mécanique Céleste”; while Herschel saw everywhere only
beginnings, possibilities of discovery, and dim prospects of “ultimate
attainments,” as to the realisation of which “it would be unwise to be
sanguine, and unphilosophical to despair” (Playfair). At the head of
very many of his chapters he might, without presumption, have written:
“Quorum pars magna fui.” They gave largely the results of his personal
investigations, and were vivified by immediate acquaintanceship
with the objects described. Hence the unsought picturesqueness of
his descriptive epithets, and the sublimity of trains of thought
communicated to him direct from the unveiled heavens.

Herschel invented in 1825, jointly with Babbage, the “astatic,” or
neutralised magnetic needle--a little instrument which was no sooner
available than it was found to be indispensable. “Nihil tetigit
quod non ornavit.” And many and various were the things touched by
his versatile genius. He had a narrow escape of becoming for life a
chemist. At the very outset of his career he applied for the vacant
chair of that science at Cambridge; but was left, as he himself
humorously expressed it, “in a glorious minority of one.” The chemical
inquiries, nevertheless, which he carried on at Slough brought to
his notice one set of relations of no trifling importance. This was
the solvent effect upon salts of silver of the hyposulphites of soda,
potash, etc. The discovery was turned to account by himself in 1840
for the “fixing” of photographic images. It secured the future of the
embryo art. By the agency of hyposulphite of soda in washing away the
unaffected chloride of silver, while leaving untouched the parts of the
deposit decomposed and darkened by exposure, permanent light-pictures,
capable of indefinite multiplication, were at length secured.

On March 14th, 1839, unaware that he had been anticipated by Fox
Talbot, Herschel presented to the Royal Society twenty-three prints
made by the sensitised paper process. A memoir communicated in 1840
was full of suggestive novelties. In it he described experiments on
“the chemical analysis of the solar spectrum,” pointing out that the
character and amount of the action exercised by the various rays
depend mainly upon the nature of the substance acted upon. He made
a start, too, with spectral photography, and his detection of the
“lavender-grey” effect to the eye of the ultra-violet section might
be said to have added a new note to the prismatic gamut. In the
opposite, or infra-red end, by simply letting the solar spectrum fall
upon a strip of paper moistened with alcohol, he detected, through the
different rates of drying where they fell, some of the “cold bands,”
by which the invisible heat-rays are furrowed. The photo-spectroscopic
apparatus devised for the purpose of these researches formed part
of the Loan Collection of Scientific Instruments exhibited at South
Kensington in 1876.

Still more essential was the improvement of substituting for paper,
glass plates spread with a sensitive film. A photograph of the old
forty-foot telescope, taken by this method in 1839, and preserved in
the South Kensington Museum, is of unrivalled antiquarian value as
regards the history of photography. The terms “positive” and “negative”
received in this remarkable paper their now familiar photographic
meaning. Its merits were acknowledged in 1840 by the award of a Royal
Medal.

Sir John Herschel would, doubtless, at that time have set aside as
a chimera the notion that the art he was engaged in promoting was
destined, in large measure, to supersede visual methods in astronomy;
that the great telescopes of the future would find their most useful
employment in concentrating the rays of celestial objects upon
sensitive plates. He soon perceived, however, the importance of
photography as an adjunct to direct observation, and recommended,
in 1847, the automatic self-registration of sun-spots. This
hint--emphasised in 1848--was acted upon in 1858, when the regular
collection of documentary evidence as to the sun’s condition was begun
at Kew with De la Rue’s “photoheliograph.”

In 1845 he published the first effective investigation of
“fluorescence,” called by him “epipolic,” or superficial, “dispersion.”
This curious phenomenon consists in the illumination to the eye of
certain substances, such as sulphate of quinine and canary glass,
under the play of _invisible_ light. Sir George Stokes showed in 1852
that the impinging rays have their undulations actually lengthened by
the action of such kinds of matter, so as to become degraded in the
spectrum, and thus brought within the range of vision.

The Herschelian theory of the sun was adopted, and long retained by
Sir John. He believed in a cool, solid interior globe sheltered by
a succession of aërial envelopes, rent, locally and temporarily,
by tornadoes of fire. The presence of inhabitants on the globe so
circumstanced was credible to him, although he abstained from dwelling
upon the advantages of their state. He carefully followed, however, the
progress of solar science, and in 1864 explained his altered views in
the _Quarterly Journal of Science_. He now regarded the sun as a wholly
gaseous mass--a conclusion in which he was anticipated only by Father
Secchi. He added that it must be largely composed of matter kept in an
intermediate condition between liquid and vaporous by “high temperature
and enormous pressure.” The spot-period, he suggested, might be that of
a revolving meteoric ring with condensations.

He was vividly interested in the “willow-leaf” controversy, raised in
1862 by Nasmyth’s misinterpreted observations. The objects seen were
simply Sir William Herschel’s “nodules”--the luminous elements of the
sun, held by Sir John in 1867 “to be permanently solid matter, having
that sort of fibrous or filamentous structure which fits them, when
juxtaposed by drifting about, and jostling one against another, to
collect in flocks as _flue_ does in a room.” He concluded with the
remarkable assertion that the sun has no real surface, “the density
diminishing from that below the photosphere to _nil_ in the higher
regions, where the pressure is _nil_.”

Herschel’s “Cape Observations” stands alone in astronomical literature
for the wide and permanent interest of its contents. They are
exceedingly various. Chapters on Halley’s Comet, on Sun-spots, the
Satellites of Saturn, Astrometry, the Constitution of the Southern
Galaxy, are associated with discussions on the nature and distribution
of nebulæ, with monographs of two, and incidental notes on many of
these enigmatical objects. The volume is illustrated with over sixty
beautiful steel engravings of nebulæ and clusters, of sun-spots, and of
the comet.

The speculations it includes regarding the nature of nebulæ, deserve
even now to be remembered. Sir John was, at the outset, an unwavering
adherent of the theory developed by his father in 1811. They were
composed, he held in 1825, of a “self-luminous; or phosphorescent
material substance, in a highly dilated or gaseous state, but gradually
subsiding, by the mutual gravitation of its molecules, into stars
and sidereal systems.” His personal experience, however, ran counter
to this view. In 1833 he had become convinced that a nebula is, in
general, “nothing more than a cluster of discrete stars.”

The successful resolution into stars, with the great Parsonstown
specula, of many nebulæ until then called irresolvable, carried him
still further in the same direction. To him, as to other thinkers,
the presence in space of a self-luminous cosmic fluid became more
than doubtful. In his Presidential Address to the British Association
in 1845, he dwelt with enthusiasm on the completion of the Rosse
reflector--“an achievement of such magnitude, that I want words to
express my admiration of it.” He regarded “as one of the grand fields
open for discovery with such an instrument, those marvellous and
mysterious bodies, or systems of bodies, the nebulæ.” Their frequent
resolution, actual or indicated, with increased optical power, led
him to attribute recalcitrance in this respect to the smallness and
closeness of the stars of which they consist; he held them, in short,
to be “optically, and not physically, nebulous.”

A new consideration was thus introduced into discussions on nebulæ. The
whole burthen of accounting for their varieties in telescopic aspect
need no longer be thrown upon differences of remoteness; diversities
in the size and closeness of nebular _molecules_ would answer the same
purpose. So that pulverulent agglomerations, it was thought, might pass
by insensible gradations into collections of truly sun-like bodies. All
distinction between nebulæ and clusters was then abolished, the members
of both classes consisting, like the sun’s photosphere, of shining
granules, supported in an obscure medium, varying in real magnitude
from _floccules_ to great globes, while each vast compound body rotated
_en masse_ on an axis. Whatever the merits of this scheme, it at least
harmonises with the now prevalent opinion that nebulæ and clusters
belong to one unbroken cosmical series. “They are divided,” Mr. Cowper
Ranyard wrote in 1893, “by no hard and fast line. The larger nebulæ may
be described as groups of stars surrounded by bright nebulosity, and
star-clusters as groups of stars surrounded by faint nebulosity.”

Herschel’s assimilation of nebulæ to clusters was not meant to apply
to “those extraordinary objects resembling the wisps and curls of a
cirrous cloud,” which confront the astronomer in Orion, Argo, and
elsewhere. “The wildest imagination,” he said, “can conceive nothing
more capricious than their forms. With their resolution,” he averred,
“and that of elliptic nebulæ, the idea of a nebulous matter, in the
nature of a shining fluid or condensible gas, would cease to derive
any support from observation.” He, in fact, discarded it absolutely on
the deceptive analysis into stars at Parsonstown and Harvard College
of the Orion and Andromeda nebulæ. The discredited hypothesis was
nevertheless triumphantly reinstated by Dr. Huggins’s spectroscopic
observations in 1864.

One-third of the whole nebular contents of the heavens Herschel found
to be collected into a broad, irregular patch, the central point of
which in Virgo coincides almost precisely with the northern pole of
the Milky Way. He compared it to a canopy surmounting the galactic
zone. In the other hemisphere the arrangement, although less distinctly
characterised, is on the same general plan. Plainly, then, nebular
distribution has an opposite correspondence with stellar distribution,
and the two partial systems are complementary one to another, Herschel,
however, contented himself with the somewhat ambiguous statement that
“the nebulous system is distinct from the sidereal, though involving
and, to a certain extent, intermixed with it.”

His verdict as to the ground-plan of the sidereal edifice might be
summed up in the phrase, “Not a stratum, but an annulus,” our own
situation being in a relatively vacant interior space. Hence, the sun
belongs, not to the Milky Way proper--as it should on the stratum
theory--but to the system of which the Milky Way forms part. This
conclusion was in itself a distinct advance towards the solution of an
exorbitantly difficult problem. The grand question as to the remoteness
of the star-clouds in that gleaming sky-girdle was definitely raised
by it; and the question is not, in the nature of things, unanswerable.
Herschel’s annulus was not a neat structure with a cylindrical
section, but “a flat ring, or some other re-entering form of immense
and irregular breadth and thickness.” It is cloven over one-third of
its circumference; it is interrupted by huge chasms; it is bent, and
shattered and broken, and probably set with tentacular appendages,
giving rise, by their foreshortening, to very complex visual effects.
All of which modifying circumstances Herschel implicitly recognised.
He was the first to gather any direct intimations of the existence
of that “solar cluster” which, guessed at by the elder Herschel, has
of late assumed a sort of elusive reality. A zone of bright stars,
including those of Orion, Canis Major, the Ship, the Cross, and the
Centaur, struck him at once as a conspicuous feature in the scenery of
the southern heavens. Its aspect led him to “suspect that our nearest
neighbours in the sidereal system form part of a subordinate sheet, or
stratum,” inclined at an angle of twenty degrees to the plane of the
Milky Way. To Dr. Gould at Cordoba, in 1879, “few celestial phenomena”
appeared “more palpable” than this projected star-belt; and, since
it traces out a great circle on the sphere, the sun must be placed
within it, and pretty accurately in its plane; yet the difficulty
of associating it intimately with our particular star seems all but
insurmountable.

Herschel’s minor and occasional writings were neither few nor
unimportant. He contributed articles on “Isoperimetrical Problems”
and “Mathematics” to Brewster’s _Edinburgh Cyclopædia_, and on
“Meteorology,” “Physical Geography,” and “The Telescope,” to the
eighth edition of the _Encyclopædia Britannica_. These last were
printed separately as well. He edited in 1849 the Admiralty “Manual
of Scientific Inquiry,” and criticised in the _Edinburgh_ and
_Quarterly Reviews_ Mrs. Somerville’s “Mechanism of the Heavens,”
Whewell’s “History of the Inductive Sciences,” Humboldt’s “Kosmos,”
and Quetelet’s “Theory of Probabilities.” His addresses as President
of the Royal Astronomical Society were models of their kind, and the
same might be said of his memoirs of Baily and Bessel in the “Monthly
Notices.” Most of them were collected in 1857, with his review
articles, into a volume of “Essays;” and his attractive “Familiar
Lectures on Scientific Subjects,” published in 1867, gave permanence to
some popular discourses delivered in the school-house of Hawkhurst, as
well as to articles from _Good Words_ on Light and other subjects. No
less than 152 papers by him are included in scientific repertories.

He had a considerable faculty for translating poetry, and its exercise
made one of his favourite recreations. Having adopted the literal
theory of the art, he kept strictly to the original metres, and thus
fettered, got over the ground with more grace and ease than might have
been expected. His first attempt with English hexameters was in a
version of Schiller’s “Walk,” privately printed in 1842. He had come
to love the poem through its association in his mind with a favourite
stroll up the side of Table Mountain; and a translation of it in the
_Edinburgh Review_ leaving, as he thought, something to be desired,
he tried his hand, and distributed the result “among his friends as
his Christmas sugar plum.” The various acknowledgments made an amusing
collection. One lady said that she “found it difficult to get into the
_step_ of the _Walk_.” Another correspondent declared that the _Walk_
had got into a _Run_ through ceaseless borrowing. A third qualified his
encomium upon the ideas by adding, “To the _verse_ I am _averse_.”
Joanna Baillie, however, and her sister were delighted with both the
substance and form of the poem, and it was included among Whewell’s
“English Hexameter Translations” in 1847.

His success encouraged him, after twenty years, to undertake an
indefinitely more difficult task. Pope’s Iliad he described happily as
“a magnificent adumbration” of the original; but he aimed rather at
producing a “fac-simile,” in

    “Hexameters no worse than daring Germany gave us.”

His version should come as near as he could bring it to a photograph
of a grand piece of architecture; and as a measure of its fidelity, he
printed in italics all the words _not_ in the text. Whewell remarked
that it was “curious to see how few he had managed to make them,” and
preferred his translation to any other with which he was acquainted.
But English hexameters were a hobby of the Master of Trinity, who
accordingly viewed with partiality what Tennyson called the “burlesque
barbarous experiment” of thus lamely rendering “the strong-wing’d music
of Homer.”

De Morgan, too, was one of the “averse.” “Many thanks for the
hexameters,” he wrote, on receiving an instalment of the Collingwood
Iliad; “they are as good as they can be, but all the logic in the
world does not make me feel them to be English metre, and they give
satisfaction only by reminding one of the Greek: just as, mark you,
a flute-player--which I have been these forty-five years--only plays
Haydn and Mozart because he has the assistance of the orchestral
accompaniment which arises in his head with the melody. The hexameter,
it is clear, does not fix itself in the popular mind. The popular mind
knows neither quantity nor accent, but that which is to last bites its
own way in, without any effort.”

Yet Herschel’s translation is not without merit. It is disfigured
neither by affectation nor by magniloquence, and it catches here and
there something of the greatness of the unapproached original. Let us
take two specimens; this from the “Shield of Achilles”:--

     “There he depicted the earth, and the canopied sky, and the ocean;
      There the unwearied sun, and the full-orb’d moon in their courses.
      All the configured stars, which gem the circuit of heaven,
      Pleiads and Hyads were there, and the giant force of Orion.
      There the revolving Bear, which the Wain they call, was
          ensculptured,
      Circling on high, and in all its course regarding Orion;
      Sole of the starry train which refuses to bathe in the Ocean.”

The next likewise appeals to the astronomer. It is the famous simile
from the end of the Eighth Book:--

     “As when around the glowing moon resplendent in ether,
      Shines forth the heavenly host, and the air reposes in stillness;
      Gleams every pointed rock, stands forth each buttress in prospect;
      Shimmers each woodland vale; and from realms of unspeakable glory
      Op’ning, the stars are revealed; and the heart of the shepherd
          rejoices.
      Such, and so many the fires, by the Trojans kindled, illumined
      Eddying Xanthus’ stream, and the ships, and the walls of the city.”

Sir John Herschel corresponded with Mr. Proctor, during the last two
years of his life, on the subject of sidereal construction; and his
replies to the arguments put before him show that his mind retained,
even then, its openness and flexibility. He had none of the contempt
for speculative excursions which sometimes walls up the thinking-powers
of observers. “In the midst of so much darkness,” he held that “we
ought to open our eyes as wide as possible to any glimpse of light,
and utilise whatever twilight may be accorded us, to make out, though
but indistinctly, the forms that surround us.” “_Hypotheses fingo_ in
this style of our knowledge,” he went on, “is quite as good a motto
as Newton’s _non fingo_--provided always they be not hypotheses as to
modes of physical action for which experience gives no warrant.” And
again: “We may--indeed, must--form theories as we go along; and they
serve as guides for inquiry, or suggestions of things to inquire; but
as yet we must hold them rather loosely, and for many years to come
keep looking out for side-lights.”

These were his last words on the philosophy of discovery: and they
constituted his last advice to scientific inquirers. But, good as
were his precepts, his example was better. There was no discrepancy
between his work and his thought. Both combined to inculcate aloofness
from prejudice, readiness of conviction in unequivocal circumstances,
suspension of judgment in dubious ones, and in all, candour, sobriety,
and an earnest seeking for truth.




INDEX.


  Actinometer, J. Herschel’s, 152, 179, 180

  Adams, J. C., at Collingwood, 188

  Ages of heavenly bodies, 68, 94, 170

  Alexander, the Czar, 49

  Amici, of Modena, 148, 150

  Apertures, method of, 61, 63

  Apex, solar, 78, 80

  Archbishop of Canterbury, and George III., 38

  Argelander, 80, 106

  Asteroids, 46, 90–1, 95, 100

  Astrometer, J. Herschel’s, 177

  Astronomical Society, 49, 152, 188

  Aubert, Alexander, 16, 101, 124


  Babbage, companionship with J. Herschel, 143–4, 149, 152;
    astatic needle, 208

  Bailey, S. I., 169, 170

  Baily, Francis, 164, 185, 186, 187

  Barnard, diameters of asteroids, 91;
    nebulosities, 110–11;
    photographs of Milky Way, 174

  Bates, Joah, anecdote of W. Herschel, 12

  Bath, centre of fashion, 12;
    Herschel’s residences there, 17, 26, 47

  Beckedorff, Mrs., 126, 127, 160;
    Miss, 138

  Bessel, solar movement, 80;
    estimate of W. Herschel, 109;
    Halley’s comet, 177;
    at Collingwood, 187;
    memoir of, 216

  Biot, estimate of J. Herschel, 201

  Bonaparte, Lucien, 33, 44

  Bonaparte, Napoleon, Herschel’s interview with, 47

  Bradley, observation of Castor, 76

  Brougham, Lord, 53, 88, 90, 207

  Burney, Dr., notices of W. Herschel, 12, 44, 45–6;
    walk through forty-foot, 38;
    notices of Caroline and J. Herschel, 125, 142

  Burney, Miss, meetings with W. Herschel, 38–9;
    with Mrs. and Miss Herschel, 44, 124, 125, 127

  Burnham, double stars, 103;
    planetary nebulæ, 155


  Campbell, Thomas, admiration for W. Herschel, 47–8;
    notice of his son, 145

  Cavendish, anecdote of, 100

  Clay Hall, 36

  Climate, changes of, 82

  Comet, of October 1806, 48;
    of 1811, 94;
    Encke’s, 124, 175;
    of 1819, 128–9;
    Biela’s, 153;
    Halley’s, 175–6, 180, 211

  Comets, decay of, 94;
    Miss Herschel’s, 124, 125

  Common, Dr., five-foot reflector, 99

  Construction of the Heavens, 53, 60, 113–114, 214–15


  Dante and the “Divina Commedia,” 15

  Datchet, house at, 32, 36

  Dawes, sun-spot nuclei, 83

  De la Rue, photoheliograph, 210

  De Morgan, letter to Captain Smyth, 188–9;
    Herschel and the coinage, 191;
    friendship with, 197;
    dislike to hexameters, 217

  Dreyer, Catalogue of Nebulæ, 192


  Easton, Milky Way structure, 106

  Edgeworth, Miss, at Slough and Collingwood, 192–3


  Feldhausen, 163, 180, 181

  Flamsteed, British Catalogue, 80, 123, 126


  Galileo, double-star method of parallaxes, 55

  Gauss, 151, 201, 205

  George III., patronage of Herschel, 10, 24, 28–9, 30, 32, 33;
    taste for astronomy, 30, 47;
    walk through great telescope, 38

  Gill, Dr., Herschel’s micrometers, 103;
    photographic catalogue, 106;
    photographs of Argo nebula, 167;
    of Omega Centauri, 169

  Gordon, Lady, portrait of Sir J. Herschel, 202

  Gould, Dr., solar cluster, 107, 215

  Grahame, James, 149

  Gravitation, extension of to stellar systems, 77, 148

  Gregorian reflectors, 20, 29

  Griesbach, Mrs., 10, 116;
    her sons, 10, 28, 29


  Halley, list of nebulæ, 19;
    stellar motions, 77

  Hamilton, Sir W. R., communications with J. Herschel, 146, 152,
          158, 173, 188;
    speech by, 182;
    at Collingwood, 193;
    quaternions, 194–5

  Haydn, visit to Slough, 44

  Heat-rays in solar spectrum, 95–6

  Herschel, Alexander, assisted his brother, 13, 21, 27, 120;
    accompanied him to Göttingen, 37;
    supported by him, 51;
    care for his sister, 118

  Herschel, Professor Alexander, meteoric researches, 201

  Herschel, Caroline, fetched to Bath, 15, 118;
    help in speculum making, 15, 20, 124;
    a singer, 21, 117, 119;
    remarks, 25, 27, 34, 49;
    letters from W. Herschel, 28, 29, 30, 129;
    household cares, 32, 118, 121;
    reminiscences, 35, 36, 37, 39, 48, 50, 68;
    annuity, 51, 131;
    birth and childhood, 115–16;
    education, 115, 118, 121;
    visits to London, 121, 127;
    discoveries of nebulæ, 122;
    of comets, 124–5, 139;
    her brother’s assistant, 122–3, 125;
    catalogues nebulæ, 123, 132;
    Index to Flamsteed’s observations, 126;
    royal attentions, 126, 127, 133, 135, 139;
    anxiety about her brother’s health, 128–9;
    return to Hanover, 130–1;
    Gold Medals bestowed on, 132, 138;
    joy in her nephew’s career, 134–5, 159;
    his visits, 135–36, 159;
    Recollections and Journals, 137, 138;
    death, 139;
    personality, 139–41;
    anecdotes of J. Herschel’s childhood, 142;
    his letters to her, 151, 152, 153, 162–3, 164, 175, 176, 187;
    her portrait, 196;
    her advice to him, 205

  Herschel, Dietrich, 20–1, 51, 127–8, 130, 131

  Herschel, Sir John, dismantling of great telescope, 43;
    catalogues of nebulæ, 132, 155, 191–2;
    visits to Hanover, 135–6, 151, 159–60, 184;
    nebular observations, 136, 153, 154–7, 165–7;
    Cape Expedition, 135, 159–2, 181–2;
    birth and childhood, 142;
    university career, 143–5;
    medals awarded to, 145, 148, 149, 157, 187, 201;
    work on double stars, 134, 146–48, 157;
    method for computing orbits, 148–9;
    general catalogue, 192;
    ascents of Monte Rosa and Etna, 149–50;
    explorations in Auvergne, 152;
    experiments on solar radiation, 151–2, 179;
    visit to Ireland, 152;
    cometary observations, 153, 175–6, 180, 189;
    telescopes, 153, 158, 164, 183;
    discovery of star in Orion-trapezium, 158;
    marriage, 159;
    Feldhausen, 163, 180–1;
    Cape climate, 164;
    Magellanic Clouds, 165–6;
    Argo nebula, 167;
    Eta Argûs, 168–9;
    globular clusters, 169–71, 213;
    star-gauging, 171–2;
    comets, 175–6;
    stellar photometry, 177;
    solar theory, 178–9, 211;
    Saturnian satellites, 180;
    magnetic work, 184, 189, 208;
    constellational reform, 185;
    removal to Collingwood, 186;
    Cape Results, 186–7, 211–12;
    President Astronomical Society, 188;
    Master of the Mint, 190–1;
    guests at Collingwood, 188, 193, 195;
    sonnet, 194;
    family life, 195–6;
    death, 197;
    powers and character, 198–201;
    books, 205–8;
    photographic experiments, 209–10;
    nature of nebulæ, 212–14;
    solar cluster, 215;
    poetical performances, 216–18;
    philosophy of discovery, 219

  Herschel, Colonel John, examination of nebular spectra, 201

  Herschel, Isaac, 9, 21, 115, 116

  Herschel, Jacob, 116, 117, 128

  Herschel, Lady, the elder, 44, 50, 152, 160

  Herschel, Lady, the younger, 159, 192, 194, 201

  Herschel, Sir William, birth, 9;
    musical career, 10–16, 21, 26, 121;
    telescope, making, 14–15, 17, 19, 20, 22;
    thirty-foot, 26–8,
    seven-foot, 28–9;
    for sale, 33;
    forty-foot, 34, 37, 38, 41–3, 49, 50, 100, 137, 210;
    twenty-foot, 35–6, 40, 50;
    front-view telescopes, 40, 41, 102, 153;
    space-penetrating power of, 61, 98;
    reviews of the heavens, 19, 20, 26, 35, 36, 42, 46;
    early papers, 22–3;
    discovery of Uranus, 24–5, 120;
    observations of double stars, 26, 49, 55–6, 75;
    interviews with the king, 28–30;
    royal astronomer, 30, 32–3;
    mode of observing, 30, 122;
    discovery of Uranian satellites, 40, 93, 153;
    of Saturnian satellites, 41, 43, 92;
    marriage, 44;
    aversion to poetry, 45–6;
    interview with Bonaparte, 47;
    observations of comets, 48, 94, 128–9;
    failure of health, 49–50, 128–9;
    death and character, 51;
    construction of the heavens, 53–4, 60, 114;
    star distances, 54–5, 57, 60–1, 64, 75;
    star-gauging, 57–8, 113;
    nature of the Milky Way, 57–9, 62–3;
    chasms in, 68;
    method of apertures, 61;
    catalogues of nebulæ, 64;
    varieties, 65;
    island universes, 66–7, 72;
    development, 67–8;
    nebulous fluid, 69–70;
    condensation into stars, 71–2, 109;
    nebular distribution, 73;
    discovery of binary stars, 76–7, 147;
    transport of the solar system, 77, 80, 108;
    stellar photometry, 80–2, 174–5;
    theory of the sun, 83–6, 211;
    sun spots and weather, 87–8;
    observations of Venus, 88;
    of Mars, 89;
    of the asteroids, 90;
    of Saturn, 91;
    law of satellite-rotation, 92;
    lunar volcanoes, 93;
    detection of infra-red heat-rays, 95–7;
    use of high powers, 101–2;
    micrometers, 103;
    photometric enumeration, 106;
    solar cluster, 107–8;
    diffused nebulosities, 110–11;
    a founder of sidereal astronomy, 112

  Herschel, Sir William J., 49, 136, 183, 201

  Huggins, Dr., spectra of nebulæ, 109, 214;
    of stars, 113

  Humboldt, 133, 138, 170, 184

  Huygens, improvement of telescopes, 17


  Jacob, southern Milky Way, 172

  Japetus, rotation of, 92

  Jupiter, trade wind theory of, 91;
    rotation of satellites, 93


  Kapteyn, solar cluster, 107

  Knipping, Mrs., 137, 138


  Lacaille, southern nebulæ, 19

  Langley, bolometer, 95;
    atmospheric absorption, 152, 179

  Laplace, 18, 47, 91, 201, 207

  Lassell, Uranian satellites, 93;
    reflectors, 99;
    observation of Mimas, 180

  Le Verrier, 187, 188

  Lexell, orbit of Uranus, 24


  Maclear, Sir Thomas, 162, 168, 176, 181

  Magellan, Von, accounts of William and Caroline Herschel, 40, 122

  Magellanic clouds, 165–6

  Magnitudes, stellar, 81, 104–5, 177

  Mars, analogy with the earth, 89

  Maskelyne, 25, 29, 76

  Mayer, Christian, satellite-stars, 75

  Mayer, Tobias, solar translation, 77, 78

  Michell, revolving stars, 75;
    solar group, 107

  Micrometer, lamp, 24, 103;
    wire, 56, 103

  Milky Way, rifts in, 50, 67–8, 173, 175, 215;
    structure, 57–59, 62, 173–4, 214–15;
    spectral peculiarity, 105;
    distance, 106, 173, 214;
    splendour in southern hemisphere, 172;
    photographic portrayal, 174–5

  Miller, Dr., 11, 12

  Mitchell, Miss, visit to Collingwood, 195–6

  Monck, stellar spectroscopic distribution, 107

  Moon, mountains of, 22, 23;
    volcanoes, 93–4.


  Nasmyth, opinion of J. Herschel, 196–7;
    solar willow leaves, 211

  Nebula, Orion, 15, 43, 65, 70, 71, 110, 111, 153, 167, 214;
    Dumb-bell, 157;
    Argo, 167;
    Andromeda, 214

  Nebulæ, catalogues, 19, 64, 123, 132, 191–2;
    discoveries, 35, 64, 122, 165;
    nature, 66, 212–4;
    development, 67, 69, 109–10;
    distribution, 73, 214

  Nebulæ, annular, 65, 157, 165

  Nebulæ, double, 72, 156

  Nebulæ, planetary, 65, 67, 71;
    spectrum, 109;
    satellites to, 155;
    colour, 165

  Nebulæ, rifted, 157

  Nebular theory, 71–2, 109

  Newton, law of gravitation, 17, 77;
    reflectors, 20, 23;
    mode of investigation, 23, 206


  Olbers, origin of asteroids, 90;
    comet of 1819, 129;
    light extinction, 174;
    visit from J. Herschel, 184

  Orange, Prince of, enquiries at Slough, 39


  Papendick, Mrs., remarks on William and Caroline Herschel, 39, 44, 125

  Peacock, Dean, 143, 194, 203

  Photography, of stellar spectra, 104, 107;
    of nebulæ, 110–11, 113, 166–7;
    star charting by, 113, 172, 199;
    of clusters, 169–70, 171;
    of solar spectrum, 209;
    of sun-spots, 210

  Photometric enumeration, 60, 106, 107, 114;
    catalogues, 80

  Photometry, stellar, 81, 104, 177;
    photographic, 105

  Piazzi, visit to Slough, 39, 150

  Pickering, E. C. and W. H., photographs of Orion nebula, 111

  Pouillet, solar radiation, 179

  Pritchard, Dr., 143, 192, 201, 204

  Proctor, star-drift, 108;
    estimate of Sir J. Herschel, 199, 200;
    correspondence with, 218


  Ranyard, A. C., changes in nebulæ, 168;
    clusters, 213

  Roberts, Dr., photographs of nebulæ, 157, 165

  Rosse reflector, 99, 212

  Russell, H. C., photographs of Magellanic clouds, 166;
    of Argo nebula, 167;
    of Milky Way, 175


  Saturn, artificial, 30;
    satellites, 41, 43, 91, 92, 180;
    rings, 91–2

  Savary, stellar orbits, 148, 149

  Schröter, 34, 84, 88–9

  Secchi, 113, 211

  See, Dr., double nebulæ, 156

  Sirius, brilliancy, 42, 168;
    standard star, 58, 61, 63, 80

  Slough, W. Herschel’s residence at, 36, 44;
    birthplace of J. Herschel, 142

  Sniadecki, stay at Slough, 39

  Solar cluster, 107, 215

  Solar radiation, 151–2, 179

  Somerville, Mrs., 132

  South, Sir James, 146, 147, 149

  Spectrum analysis, 84, 204, 209

  Spencer, unity of sidereal system, 166

  Stanley, Dean, on J. Herschel, 199

  Star-clusters, 49, 59, 63, 67, 72, 169–71, 213

  Star-gauging, 57–8, 113, 171–2

  Stars, binary, 72, 156;
    discovery, 76–7, 147;
    orbits, 147–9

  Stars, double, observations of, 55–6, 103, 146–8, 157;
    colours, 56, 112, 156;
    nebular relations, 155

  Stars, distribution of, 58–9, 60, 73, 81, 106, 171–2

  Stars, movements of, 77, 107–8

  Stars, nebulous, 69, 70, 71

  Stars, spectra of, 83, 105

  Stars, spectroscopic binary, 104

  Stars, temporary, 66–7

  Stars, variable, 23, 81–2, 168–9

  Stokes, Sir G., fluorescence, 210

  Stone, Herschel’s assistant, 180

  Struve, W., 148, 158, 188

  Sun, translation, 77–80, 108;
    vicissitudes, 82, 87, 88;
    constitution, 83–6, 178–9, 211

  Sussex, Duke of, 158


  Telescopes, Improvement of, 17, 19, 20, 24–6, 33, 36, 98–100


  Uranus, discovery of, 24–5, 26, 120;
    satellites, 40, 93, 153


  Watson, Sir W., 16, 22, 27, 30, 47, 124

  Watt, James, 47

  Whewell, Dr., unity of sidereal system, 76, 166;
    friendship with J. Herschel, 145, 163, 191, 200;
    tidal data, 181;
    articles in Quarterly Review, 186, 205–6;
    Geological Society, 189;
    on optical enquiries, 203–4;
    hexameters, 217

  Wolf, Dr. Max, photographs of nebulæ, 111;
    of Milky Way, 175

  Wollaston, 145, 177

  Worlds, inhabited, 85, 86, 89, 147.


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