A POPULAR HISTORY OF ASTRONOMY DURING THE NINETEENTH CENTURY
* * * * *
BY THE SAME AUTHOR
PROBLEMS IN ASTROPHYSICS. Demy 8vo., cloth. Containing over 100 Illustrations. Price 20s. net.
THE SYSTEM OF THE STARS. Second Edition. Thoroughly revised and largely rewritten. Containing numerous and new Illustrations. Demy 8vo., cloth. Price 20s. net.
MODERN COSMOGONIES. Crown 8vo., cloth. Price 3s. 6d. net.
A. AND C. BLACK, SOHO SQUARE, LONDON, W.
* * * * *
[Illustration: THE GREAT NEBULA IN ORION, 1883
_See p. 408_]
A POPULAR HISTORY OF ASTRONOMY DURING THE NINETEENTH CENTURY
by
AGNES M. CLERKE
[Illustration: JUPITER 1879
SATURN 1885]
London Adam and Charles Black 1908
First Edition, Post 8vo., published 1885 Second Edition, Post 8vo., published 1887 Third Edition, Demy 8vo., published 1893 Fourth Edition, Demy 8vo., published 1902 Fourth Edition, Post 8vo., reprinted February, 1908
PREFACE TO THE FOURTH EDITION
Since the third edition of the present work issued from the press, the nineteenth century has run its course and finished its record. A new era has dawned, not by chronological prescription alone, but to the vital sense of humanity. Novel thoughts are rife; fresh impulses stir the nations; the soughing of the wind of progress strikes every ear. "The old order changeth" more and more swiftly as mental activity becomes intensified. Already many of the scientific doctrines implicitly accepted fifteen years ago begin to wear a superannuated aspect. Dalton's atoms are in process of disintegration; Kirchhoff's theorem visibly needs to be modified; Clerk Maxwell's medium no longer figures as an indispensable factotum; "absolute zero" is known to be situated on an asymptote to the curve of cold. Ideas, in short, have all at once become plastic, and none more completely so than those relating to astronomy. The physics of the heavenly bodies, indeed, finds its best opportunities in unlooked-for disclosures; for it deals with transcendental conditions, and what is strange to terrestrial experience may serve admirably to expound what is normal in the skies. In celestial science especially, facts that appear subversive are often the most illuminative, and the prospect of its advance widens and brightens with each divagation enforced or permitted from the strait paths of rigid theory.
This readiness for innovation has undoubtedly its dangers and drawbacks. To the historian, above all, it presents frequent occasions of embarrassment. The writing of history is a strongly selective operation, the outcome being valuable just in so far as the choice what to reject and what to include has been judicious; and the task is no light one of discriminating between barren speculations and ideas pregnant with coming truth. To the possession of such prescience of the future as would be needed to do this effectually I can lay no claim; but diligence and sobriety of thought are ordinarily within reach, and these I shall have exercised to good purpose if I have succeeded in rendering the fourth edition of _A Popular History of Astronomy during the Nineteenth Century_ not wholly unworthy of a place in the scientific literature of the twentieth century.
Table of contents (by pages)
- 1: A Popular History of Astronomy During the Nineteen
- 2: Constituted the sum and substance of astronomy
- 3: Director of the Washburn Observatory
- 4: A Popular History of Astronomy During the Nineteen
- 5: A Popular History of Astronomy During the Nineteen
- 6: A Popular History of Astronomy During the Nineteen
- 7: 1901 Taken at the Royal Observatory
- 8: Theory and observation mutually act and react
- 9: The computations of astronomers
- 10: Started by Von Zach in the year 1800
- 11: The process has included astronomy
- 12: And Mayer actually attempted the analysis
- 13: 7 the picture of sidereal science
- 14: In 1772 he hired a small telescope
- 15: And installed as Royal Astronomer
- 16: To the successful determination of the parallax of 61 Cygni
- 17: Its advantages were not lost upon Herschel
- 18: Eta Lyrae was noted as a double double star
- 19: But since the distance of Sirius
- 20: To spots without a trace of stellar formation
- 21: Contain a nebulosity of the milky kind
- 22: Herschel's theory still holds the field
- 23: Footnote 10 Caroline Lucretia Herschel
- 24: Footnote 12 Memoir of Caroline Herschel
- 25: Footnote 41 Mathemata Astronomica
- 26: With which Bradley had done his incomparable work
- 27: And presented the work to Olbers
- 28: And it was this which Bessel undertook and carried through
- 29: Thus astronomy became a truly universal science
- 30: This was an orphan lad of fourteen named Joseph Fraunhofer
- 31: 71 He then had his heliometer taken down and repaired
- 32: Small parallaxes have been determined
- 33: The determination of parallax leads
- 34: It was confirmed five years later by the younger Struve
- 35: They extended to Procyon in 1840
- 36: While in the act of trying a new 18 inch refractor
- 37: Which left the famous Dorpat telescope far behind
- 38: Sir William Herschel had but one legitimate successor
- 39: Especially in the case of Nubecula Minor
- 40: Towards the close of his residence at Feldhausen
- 41: FOOTNOTES Footnote 58 Bessel
- 42: And by Winnecke a parallax of O
- 43: Footnote 107 Stellarum Fixarum
- 44: Under the title of Austriaca Sidera by Father Malapertius
- 45: The surrounding penumbrae representing shoals or sandbanks
- 46: Its surface diversified with mountains and valleys
- 47: Like all successful innovations
- 48: Hurricanes and tornadoes prevail
- 49: Mere scrutiny of the solar surface
- 50: And was observed by Baily at Inch Bonney
- 51: Pavia contains many thousand inhabitants
- 52: Was shortsighted could distinguish
- 53: As a regular feature of total eclipses
- 54: The aureola round the eclipsed sun
- 55: After the great eclipse of 1860
- 56: FOOTNOTES Footnote 131 Kosmos
- 57: The circulus solis of course signifies the corona
- 58: The zone in which each planet moved was
- 59: Giuseppe Piazzi was born at Ponte in the Valtelline
- 60: The second by Olbers himself in Virgo
- 61: To launch the asteroidal fragments on their respective paths
- 62: The indefatigable computating partner of Laplace
- 63: 1843 ceased to breathe and to calculate
- 64: And on the 9th of July he wrote to Professor Challis
- 65: And Neptune's vast distance of 2
- 66: William Lassell was a brewer by profession
- 67: Into one encircling ring by Huygens in 1655
- 68: No further Neptunian or Uranian satellites can be perceived
- 69: In a letter to Von Zach of June 24
- 70: And Halley accordingly fixed its return for 1758 9
- 71: Or observed the cometary visitants of northern skies
- 72: Encke became an astronomer because he was a mathematician
- 73: No great comet is of the planetary kind
- 74: Have been perceived in other comets
- 75: The stars of the cluster being visible through the comet
- 76: Both were again seen by him in unmistakable cometary shape
- 77: 260 Biela's is not the only vanished comet
- 78: Of which Zoellner 271 regarded Olbers as the founder
- 79: Was very clearly anticipated by Olbers
- 80: Issued from the nucleus towards the sun
- 81: On the 3rd of March it measured 25 deg
- 82: That of the comet of 1843 reached
- 83: Seem to mark a stage in cometary decay
- 84: Footnote 252 Mecanique Celeste
- 85: Footnote 277 Celestial Objects
- 86: Did the reflecting telescope come
- 87: And turned it into a front view reflector
- 88: For by the examination with strong lenses of an object which
- 89: He bought some land near Les Brenets
- 90: Known as Lord Oxmantown until 1841
- 91: At times the very crucibles in which his specula were cast
- 92: Yielded at once to the Parsonstown reflector
- 93: 330 The class of spiral nebulae included
- 94: The second that of the equatoreal
- 95: He employed the crossed axes of the true equatoreal
- 96: There is no once for all in astronomy
- 97: Footnote 324 Lord Rosse in Phil
- 98: Footnote 337 Miscellaneous Works
- 99: Through the genius and energy of Gauss
- 100: The ascent from minimum to maximum being
- 101: He studied the spectrum of burning spirits
- 102: He thereupon perceived that the spectrum
- 103: Discovered by Fraunhofer in 1815
- 104: Are certainly solar constituents
- 105: Equally to Kirchhoff and Bunsen
- 106: That Kirchhoff was unacquainted
- 107: Which accordingly form an interrupted spectrum
- 108: 402 What Kepler dreamed of and groped after
- 109: It will doubtless perform much more
- 110: Footnote 360 Neue Untersuchungen
- 111: Footnote 377 Annalen der Physik
- 112: As Father Secchi 408 concluded from his long experience
- 113: While the Redhill Observatory was in course of erection
- 114: These were the law of the sun's rotation
- 115: Individual equatorial spots are not uncommon
- 116: Included in his great memoir On the Solar Spectrum
- 117: The solar system of circulation
- 118: That the photosphere is a surface of condensation
- 119: A solar daguerreotype was taken at Paris
- 120: 137 instances of spots accompanied by faculae
- 121: A spectroscope of exceptionally high dispersive power
- 122: For two portions of the photosphere 123 miles apart
- 123: A magnetic storm of unparalleled intensity
- 124: 1892 the largest ever recorded at Greenwich
- 125: Maxima of one order are superposed upon
- 126: Into granules not above 100 miles in diameter
- 127: Footnote 415 Observations at Redhill
- 128: Footnote 422 Observations at Redhill
- 129: Contributions to Solar Physics
- 130: Footnote 486 Mittheilungen ueber die Sonnenflecken
- 131: And Father Secchi his six inch Cauchoix refractor
- 132: By Tennant and Janssen at Guntoor
- 133: The advantage of a prolonged eclipse
- 134: To resolve the Fraunhofer line 1474 into a pair
- 135: And the familiar one of the dark line solar spectrum
- 136: And at least the lower part of the corona
- 137: As the groundwork of the corona
- 138: To diffused chromospheric light
- 139: And rapidly diffused all round the globe
- 140: He was accompanied from Meudon by Trouvelot
- 141: And incumbent upon the chromosphere
- 142: To a distance of two or three diameters of the solar disc
- 143: But Tacchini first drew particular attention to them
- 144: Were the filaments and the streamers
- 145: 572 entangled amidst coronal streamers
- 146: The corona of 1898 presented a mixed aspect
- 147: The meteorological forecast was dubious
- 148: A critical experiment made by Ebert in 1895 served
- 149: FOOTNOTES Footnote 512 Vierteljahrsschrift Astr
- 150: Footnote 567 Professor Holden concluded
- 151: Foremost among these were Lockyer in England
- 152: To greater heights than hydrogen itself
- 153: And quite apart from the chromosphere
- 154: Taken with the Spectroheliograph of the Kenwood Observatory
- 155: 621 Another peculiarity of the chromosphere
- 156: So far Doppler was altogether right
- 157: Made with a fine diffraction spectroscope
- 158: The shortest of which belongs to the faculae
- 159: While uprushes have been witnessed by Respighi
- 160: Spectroscopically and chemically
- 161: Giving a still more complex spectrum
- 162: The infra red part of the spectrum
- 163: The agreement was verified by Angstrom
- 164: It may just balance absorption by emission
- 165: Footnote 613 Wiedemann's Annalen der Physik
- 166: Hippolyte Fizeau died in September
- 167: Footnote 669 Published in Astroph
- 168: Footnote 680 Berlin Abhandlungen
- 169: Platinum and diamond become rapidly vaporised
- 170: Substituting Dulong and Petit's for Newton's law
- 171: At a photospheric temperature of 7
- 172: Of the violet rays escape at the edge of the solar disc
- 173: And the indications of the bolometer
- 174: And a solar constant of four calories
- 175: Footnote 700 Results of Astr
- 176: Footnote 739 Annals of the Smithsonian Astroph
- 177: But Picard's result was just half Flamsteed's parallax 20
- 178: Into apparent or parallactic displacements
- 179: But takes some short time in transmission
- 180: A transit of Venus was fast approaching
- 181: In the action of a cosmopolitan observing machine
- 182: And held any parallax less than 8
- 183: Galle deduced a solar parallax of 8
- 184: Only heliometers were employed
- 185: The Germans and Belgians trusted to the heliometer
- 186: Abregee de la Parallaxe du Soleil
- 187: Footnote 773 Transits of Venus
- 188: He settled a few years later at Lilienthal
- 189: And it lasted throughout the transit
- 190: Strictly analogous to those of the moon
- 191: Denning in 1882 rotation in about twenty five hours
- 192: A physician residing at Orgeres
- 193: As a ruddy star with a minute planetary disc
- 194: 859 while an object near the northern horn of the crescent
- 195: 868 Such a dissimilarity probably exists
- 196: That full earth light on Venus
- 197: Identified Horrebow's satellite with Theta Librae
- 198: Rotate upon its axis of figure
- 199: Must have undergone extensive glaciation
- 200: Geodetical methods are unquestionably to be preferred
- 201: A very persistent lunar feature
- 202: Oder allgemeine vergleichende Selenographie
- 203: Linne had been known to Lohrmann and Maedler
- 204: Schroeter's description of Linne
- 205: In getting measures of a lunar heat spectrum
- 206: The terrestrial orbit will close in at the sides
- 207: Conclusions were reached by William Ferrel of Allensville
- 208: Footnote 813 Neueste Beytraege
- 209: Footnote 841 Bothkamp Beobachtungen
- 210: Footnote 881 Bothkamp Beobachtungen
- 211: Footnote 919 Outlines of Astr
- 212: Depending on the earth's rotation
- 213: Footnote 959 Dynamik des Himmels
- 214: Hence Bakhuyzen's period of 24h
- 215: Reach the eye of a Martian or lunar observer
- 216: Director of the Milan Observatory
- 217: 1001 with the great Lick refractor
- 218: Pickering were a number of lakes
- 219: The albedo of Mars is put by Mueller at 0
- 220: Its originator proved to be unique among asteroids
- 221: When the number of known asteroids was only eighty eight
- 222: Assigned to Vesta a diameter of 319 miles
- 223: Terrestrial analogies held their ground
- 224: Only since it was adopted and enforced by Zoellner in 1865
- 225: Perceived in 1891 by Schaeberle and Campbell
- 226: 000 from his bulging equatorial surface
- 227: Elvins of Toronto has pointed out
- 228: Of the apparent disc was inferred
- 229: And indicated a fluid formation
- 230: The brightest parts of these appendages
- 231: 38 radii of Saturn from his centre
- 232: Though almost necessarily inferred to be equatorial
- 233: In lieu of the reflected Fraunhofer lines
- 234: Almost simultaneously with Forbes
- 235: Annals of the Lowell Observatory
- 236: Footnote 1038 Spectra der Planeten
- 237: Footnote 1052 Sitzungsberichte
- 238: An Original Theory of the Universe
- 239: Footnote 1124 Comptes Rendus
- 240: As this atmosphere or nebula cooled
- 241: Mayer looked round for an alternative
- 242: It was developed with his usual ability by Lord Kelvin
- 243: 250 millionth part of the solar radiations
- 244: But to supersede that of Laplace
- 245: As a consequence of tidal friction
- 246: Consistent with spheroidal equilibrium
- 247: They showed that the lunar terrestrial system
- 248: Phobos should have been precipitated upon its surface
- 249: Variously modified and variously prevailing
- 250: Footnote 1163 Comptes Rendus
- 251: Attained its full development only after perihelion
- 252: And reaching to a still greater distance from the nucleus
- 253: A golden yellow planetary disc
- 254: And even caused Chladni temporarily to renounce his
- 255: As the result of the star fall of 1833
- 256: An alternative was proposed by Adolf Erman of Berlin in 1839
- 257: Before the close of the year 1866
- 258: And probably solid parts of comets
- 259: While the Leonids rush to meet it
- 260: Biela touched earth November 27
- 261: Was visited on November 23 by a genuine Andromede shower
- 262: We can no longer count upon the Leonids
- 263: A ball of fire was precipitated from the sky at Mazapil
- 264: With the cometary radiant for its central point
- 265: All five would show universally in cometary spectra
- 266: Footnote 1195 Comptes Rendus
- 267: Footnote 1230 In Schiaparelli's opinion
- 268: And resumed on the apparition of Donati's comet
- 269: That comets are divisible into groups
- 270: To this question Bredikhine supplied
- 271: By its first perihelion passage
- 272: Besides those of 1843 and 1880
- 273: Ascending from Auriga through Camelopardus
- 274: The chemical intensity of cometary light is
- 275: Cometary photography came to its earliest fruition with it
- 276: Otherwise the spectrum was strongly continuous
- 277: Finlay of the Cape Observatory
- 278: Just before its final rush past perihelion on September 17
- 279: For the perihelion distance of the comet of 1882
- 280: Of six or eight distinct cometary masses within 6 deg
- 281: Carbon bands had died out with approach to perihelion
- 282: It passed perihelion January 25
- 283: There was no connecting nebulosity between these objects
- 284: Enveloped in a thin nebulous husk
- 285: FOOTNOTES Footnote 1267 Astr
- 286: Footnote 1276 Annales de l'Obs
- 287: Footnote 1322 Vierteljahrsschrift Astr
- 288: Footnote 1355 Harvard Annals
- 289: The effective founders of stellar spectroscopy
- 290: Their spectra are quite closely similar to that of sunlight
- 291: Certain spectroscopic coincidences
- 292: Both show bright lines of hydrogen and helium
- 293: First noticed by Von Gothard in 1882
- 294: Thirty two Wolf Rayet stars were investigated
- 295: Sir William Huggins acted as pioneer
- 296: Rydberg's indication of the Wolf Rayet blue band at Lambda 4
- 297: An objective prism eight inches square was attached
- 298: It was first executed by Sir William Huggins early in 1868
- 299: In spectrograms of Zeta Ursae Majoris Mizar
- 300: Now it is evident that a spectroscopic binary
- 301: A new Catalogue of Variable Stars
- 302: The spectroscope had not then been invented
- 303: Become transformed into a planetary nebula
- 304: Max Wolf took a photograph of the region about Chi Aurigae
- 305: By Sir William and Lady Huggins
- 306: When last examined at Tulse Hill
- 307: Nova Carinae and Nova Centauri lit up in 1895
- 308: The nebular ray wave length 5
- 309: Spectrographic prints of the Andromeda nebula
- 310: Burnham with the Lick refractor in 1891
- 311: By the nebula and the chief stars in the constellation Orion
- 312: One of the great Andromeda nebula
- 313: With a refractor of only ten inches aperture
- 314: Be reckoned as genuine Pleiades
- 315: He resolved to employ photography for the purpose
- 316: From the reobservation of which
- 317: His parallax for Alpha Lyrae 0
- 318: The subject of his initial experiment was 61 Cygni
- 319: Burnham is beyond question the foremost
- 320: His photometric catalogue of 4
- 321: Modelled on the visual photometry of 1884
- 322: Galactic rather than solar affinities
- 323: One of these strange galactic landscapes is reproduced
- 324: Stars are bound together by twos
- 325: Footnote 1375 Spectre Solaire
- 326: Footnote 1422 Harvard Circulars
- 327: Footnote 1441 Sitzungsberichte
- 328: Footnote 1466 System of the Stars
- 329: The theories on the subject of M
- 330: Footnote 1543 Comptes Rendus
- 331: Footnote 1571 Reproduced in Astroph
- 332: Footnote 1597 Annals Cape Observatory
- 333: The colossal Rosse reflector still marks
- 334: Newall to the University of Cambridge
- 335: Such as the Lick and Yerkes refractors
- 336: Together with a chemically corrected 24 inch refractor
- 337: A site for the new observatory
- 338: And the coude or bent equatoreal has been
- 339: Loewy has realised has been felt by others
- 340: The whole visible spectrum can now be photographed
- 341: Who initiated the study of the diffraction spectrum
- 342: To be bounded by the solar system
- 343: Footnote 1644 Harvard Circulars
- 344: March 28 Discovery of Pallas by Olbers
- 345: 1829 The Koenigsberg heliometer mounted
- 346: 19 Simultaneous discovery of Hyperion by Bond and Lassell
- 347: Spectrum of prominences observed
- 348: 22 Perihelion of Schaeberle's comet
- 349: 17 Perihelion of Great Comet
- 350: 8 Roberts's photograph of the Pleiades nebulosities
- 351: First photographs of the Milky Way taken by Barnard
- 352: November McClean Spectrographs of the High and Low Sun
- 353: Among them a solar parallax 8
- 354: Reversing layer photographed by Shackleton
- 355: 21 Inauguration of the Yerkes Observatory
- 356: 22 Nova Persei discovered by Anderson
- 357: Gallium by Hartley and Ramage in 1899
- 358: Aperture in Focal Length Constructor
- 359: National 48 Martin
- 360: Royal T
- 361: Nice Gautier
- 362: Royal Sir H
- 363: 18 n
- 364: 1 1872 Lord Crawford
- 365: 13
- 366: All are provided with 13 inch photographic
- 367: 391 Altitude and azimuth instrument
- 368: Exterior Pleiades nebulosities
- 369: Magnetic and solar disturbances
- 370: Discovery of spectrum analysis
- 371: Photographic discovery of a comet
- 372: Photographs of Andromeda nebula
- 373: Hydrogen spectrum in prominences
- 374: Rotation of Jupiter's satellites
- 375: Double star method of parallaxes
- 376: Invention of achromatic telescope
- 377: Rotation of Jupiter's satellites
- 378: Photograph of Uranian spectrum
- 379: Spectroscopic observations of prominences
- 380: Spectroscopic effects of solar rotation
- 381: Refrangibility changed by movement
- 382: Revolutions of Neptune's satellite
- 383: Solar parallax from disturbed motion
- 384: Disturbance of Neptune's satellite
- 385: Of stellar and nebular spectra
- 386: Photographic celestial surveys
- 387: Spectroscopic method of observing
- 388: Discovery of Procyon's satellite
- 389: Observations of Jupiter's satellites
- 390: Transits of Jupiter's satellites
- 391: Prevision of spectrum analysis
- 392: Reversal of Fraunhofer spectrum
- 393: Polariscopic coronal photography
- 394: Exterior nebulosities of Pleiades
- 395: In preparing the Second Edition
- 396: Problems in Astrophysics looks to the future
- 397: Published by adam charles black
