Chapter XIII: The Nineteenth Century (3)
319. An entirely new contribution to the problem has resulted from certain discoveries as to the nature of heat, culminating in the recognition (about 1840-50) of heat as only one form of what physicists now call =energy=, which manifests itself also in the motion of bodies, in the separation of bodies which attract one another, as well as in various electrical, chemical, and other ways. With this discovery was closely connected the general theory known as the =conservation of energy=, according to which energy, though capable of many transformations, can neither be increased nor decreased in quantity. A body which, like the sun, is giving out heat and light is accordingly thereby losing energy, and is like a machine doing work; either then it is receiving energy from some other source to compensate this loss or its store of energy is diminishing. But a body which goes on indefinitely giving out heat and light without having its store of energy replenished is exactly analogous to a machine which goes on working indefinitely without any motive power to drive it; and both are alike impossible.
The results obtained by John Herschel and Pouillet in 1836 (§ 307) called attention to the enormous expenditure of the sun in the form of heat, and astronomers thus had to face the problem of explaining how the sun was able to go on radiating heat and light in this way. Neither in the few thousand years of the past covered by historic records, nor in the enormously great periods of which geologists and biologists take account, is there any evidence of any important permanent alteration in the amount of heat and light received annually by the earth from the sun. Any theory of the sun’s heat must therefore be able to account for the continual expenditure of heat at something like the present rate for an immense period of time. The obvious explanation of the sun as a furnace deriving its heat from combustion is found to be totally inadequate when put to the test of figures, as the sun could in this way be kept going at most for a few thousand years. The explanation now generally accepted was first given by the great German physicist _Hermann von Helmholtz_ (1821-1894) in a popular lecture in 1854. The sun possesses an immense store of energy in the form of the mutual gravitation of its parts; if from any cause it shrinks, a certain amount of gravitational energy is necessarily lost and takes some other form. In the shrinkage of the sun we have therefore a possible source of energy. The precise amount of energy liberated by a definite amount of shrinkage of the sun depends upon the internal distribution of density in the sun, which is uncertain, but making any reasonable assumption as to this we find that the amount of shrinking required to supply the sun’s expenditure of heat would only diminish the diameter by a few hundred feet annually, and would therefore be imperceptible with our present telescopic power for centuries, while no earlier records of the sun’s size are accurate enough to shew it. It is easy to calculate on the same principles the amount of energy liberated by a body like the sun in shrinking from an indefinitely diffused condition to its present state, and from its present state to one of assigned greater density; the result being that we can in this way account for an expenditure of sun-heat at the present rate for a period to be counted in millions of years in either past or future time, while if the rate of expenditure was less in the remote past or becomes less in the future the time is extended to a corresponding extent.
No other cause that has been suggested is competent to account for more than a small fraction of the actual heat-expenditure of the sun; the gravitational theory satisfies all the requirements of astronomy proper, and goes at any rate some way towards meeting the demands of biology and geology.
If then we accept it as provisionally established, we are led to the conclusion that the sun was in the past larger and less condensed than now, and by going sufficiently far back into the past we find it in a condition not unlike the primitive nebula which Laplace presupposed, with the exception that it need not have been hot.
320. A new light has been thrown on the possible development of the earth and moon by Professor G. H. Darwin’s study of the effects of tidal friction (cf. § 287 and §§ 292, 293). Since the tides increase the length of the day and month and gradually repel the moon from the earth, it follows that in the past the moon was nearer to the earth than now, and that tidal action was consequently much greater. Following out this clue. Professor Darwin found, by a series of elaborate calculations published in 1879-81, strong evidence of a past time when the moon was close to the earth, revolving round it in the same time in which the earth rotated on its axis, which was then a little over two hours. The two bodies, in fact, were moving as if they were connected; it is difficult to avoid the probable inference that at an earlier stage the two really were one, and that the moon is in reality a fragment of the earth driven off from it by the too-rapid spinning of the earth, or otherwise.
Professor Darwin has also examined the possibility of explaining in a similar way the formation of the satellites of the other planets and of the planets themselves from the sun, but the circumstances of the moon-earth system turn out to be exceptional, and tidal influence has been less effective in other cases, though it gives a satisfactory explanation of certain peculiarities of the planets and their satellites. More recently (1892) Dr. _See_ has applied a somewhat similar line of reasoning to explain by means of tidal action the development of double stars from an earlier nebulous condition.
Speaking generally, we may say that the outcome of the 19th century study of the problem of the early history of the solar system has been to discredit the details of Laplace’s hypothesis in a variety of ways, but to establish on a firmer basis the general view that the solar system has been formed by some process of condensation out of an earlier very diffused mass bearing a general resemblance to one of the nebulae which the telescope shews us, and that stars other than the sun are not unlikely to have been formed in a somewhat similar way; and, further, the theory of tidal friction supplements this general but vague theory, by giving a rational account of a process which seems to have been the predominant factor in the development of the system formed by our own earth and moon, and to have had at any rate an important influence in a number of other cases.
AUTHORITIES AND BOOKS FOR STUDENTS.
I. GENERAL.
I have made great use throughout of R. Wolf’s _Geschichte der Astronomie_, and of the six volumes of Delambre’s _Histoire de l’Astronomie_ (_Ancienne_, 2 vols.; _du Moyen Age_, 1 vol.; _Moderne_, 2 vols.; _du Dixhuitième Siècle_, 1 vol.). I shall subsequently refer to these books simply as _Wolf_ and _Delambre_ respectively. I have used less often the astronomical sections of Whewell’s _History of the Inductive Sciences_ (referred to as _Whewell_), and I am indebted—chiefly for dates and references—to the histories of mathematics written respectively by Marie, W. W. R. Ball, and Cajori, to Poggendorff’s _Handwörterbuch der Exacten Wissenschaften_, and to articles in various biographical dictionaries, encyclopaedias, and scientific journals. Of general treatises on astronomy Newcomb’s _Popular Astronomy_, Young’s _General Astronomy_, and Proctor’s _Old and New Astronomy_ have been the most useful for my purposes.
It is difficult to make a selection among the very large number of books on astronomy which are adapted to the general reader. For students who wish for an introductory account of astronomy the Astronomer Royal’s _Primer of Astronomy_ may be recommended; Young’s _Elements of Astronomy_ is a little more advanced, and Sir R. S. Ball’s _Story of the Heavens_, Newcomb’s _Popular Astronomy_, and Proctor’s _Old and New Astronomy_ enter into the subject in much greater detail. Young’s _General Astronomy_ may also be recommended to those who are not afraid of a little mathematics. There are also three modern English books dealing generally with the history of astronomy, in all of which the biographical element is much more prominent than in this book: viz. Sir R. S. Ball’s _Great Astronomers_, Lodge’s _Pioneers of Science_, and Morton’s _Heroes of Science: Astronomers_.
II. SPECIAL PERIODS.
_Chapters I. and II._—In addition to the general histories quoted above—especially _Wolf_—I have made most use of Tannery’s _Recherches sur l’Histoire de l’Astronomie Ancienne_ and of several biographical articles (chiefly by De Morgan) in Smith’s _Dictionary of Classical Biography and Mythology_. Ideler’s _Chronologische Untersuchungen_, Hankel’s _Geschichte der Mathematik im Alterthum und Mittelalter_, G. C. Lewis’s _Astronomy of the Ancients_, and Epping & Strassmaier’s _Astronomisches aus Babylon_ have also been used to some extent. Unfortunately my attention was only called to Susemihl’s _Geschichte der Griechischen Litteratur in der Alexandriner Zeit_ when most of my book was in proof, and I have consequently been able to make but little use of it.
I have in general made no attempt to consult the original Greek authorities, but I have made some use of translations of Aristarchus, of the _Almagest_, and of the astronomical writings of Plato and Aristotle.
_Chapter III._—The account of Eastern astronomy is based chiefly on Delambre, and on Hankel’s _Geschichte der Mathematik im Alterthum und Mittelalter_; to a less extent on Whewell. For the West I have made more use of Whewell, and have borrowed biographical material for the English writers from the _Dictionary of National Biography_. I have also consulted a good many of the original astronomical books referred to in the latter part of the chapter.
I know of no accessible book in English to which to refer students except _Whewell_.
_Chapter IV._—For biographical material, for information as to the minor writings, and as to the history of the publication of the _De Revolutionibus_ I have used little but Prowe’s elaborate _Nicolaus Coppernicus_, and the documents printed in it. My account of the _De Revolutionibus_ is taken from the book itself. The portrait is taken from Dandeleau’s engraving of a picture in Lalande’s possession. I have not been able to discover any portrait which was clearly made during Coppernicus’s lifetime, but the close resemblance between several portraits dating from the 17th century and Dandeleau’s seems to shew that the latter is substantially authentic.
There is a readable account of Coppernicus, as well as of several other astronomers, in Bertrand’s _Fondateurs de l’Astronomie Moderne_; but I have not used the book as an authority.
_Chapter V._—For the life of Tycho I have relied chiefly on Dreyer’s _Tycho Brahe_, which has also been used as a guide to his scientific work; but I have made constant reference to the original writings: I have also made some use of Gassendi’s _Vita Tychonis Brahe_. The portrait is a reproduction of a picture in the possession of Dr. Crompton of Manchester, described by him in the _Memoirs of the Manchester Literary and Philosophical Society_, Vol. VI., Ser. III. For minor Continental writers I have used chiefly _Wolf_ and _Delambre_, and for English writers, _Whewell_, various articles by De Morgan quoted by him, and articles in the _Dictionary of National Biography_.
Students will find in Dreyer’s book all that they are likely to want to know about Tycho.
_Chapter VI._—For Galilei’s life I have used chiefly Karl von Gebler’s _Galilei und die Römische Curie_, partly in the original German form and partly in the later English edition (translated by Mrs. Sturge). For the disputed questions connected with the trial I have relied as far as possible on the original documents preserved in the Vatican, which have been published by von Gebler and independently by L’Épinois in _Les Pièces du Procès de Galilée_: in the latter book some of the most important documents are reproduced in facsimile. For personal characteristics I have used the charming _Private Life of Galileo, compiled chiefly from his correspondence and that of his daughter Marie Céleste_. I have also read with great interest the estimate of Galilei’s work contained in H. Martin’s _Galilée_, and have probably borrowed from it to some extent. What I have said about Galilei’s scientific work has been based almost entirely on study of his own books, either in the original or in translation: I have used freely the translations of the _Dialogue on the Two Chief Systems of the World_ and of the _Letter to the Grand Duchess Christine_ by Salusbury, that of the _Two New Sciences_ by Weston (as well as that by Salusbury), and that of the _Sidereal Messenger_ by Carlos. I have also made some use of various controversial tracts written by enemies of Galilei, which are to be found (together with his comments on them) in the magnificent national edition of his works now in course of publication; and of the critical account of Galilei’s contributions to dynamics contained in Mach’s _Geschichte der Mechanik_.
_Wolf_ and _Delambre_ have only been used to a very small extent in this chapter, chiefly for the minor writers who are referred to.
The portrait is a reproduction of one by Sustermans in the Uffizi Gallery.
There is an excellent popular account of Galilei’s life and work in the _Lives of Eminent Persons_ published by the Society for the Diffusion of Useful Knowledge; students who want fuller accounts of Galilei’s life should read Gebler’s book and the _Private Life_, which have been already quoted, and are strongly recommended to read at any rate parts of the _Dialogue on the Two Chief Systems of the World_, either in the original or in the picturesque old translation by Salusbury: there is also a modern German version of this book, as well as of the _Two New Sciences_, in Ostwald’s series of _Klassiker der exakten Wissenschaften_.
_Chapter VII._—For Kepler’s life I have used chiefly _Wolf_ and the life—or rather biographical material—given by Frisch in the last volume of his edition of Kepler’s works, also to a small extent Breitschwerdt’s _Johann Keppler_. For Kepler’s scientific discoveries I have used chiefly his own writings, but I am indebted to some extent to _Wolf_ and _Delambre_, especially for information with regard to his minor works. The portrait is a reproduction of one by Nordling given in Frisch’s edition.
The _Lives of Eminent Persons_, already referred to, also contains an excellent popular account of Kepler’s life and work.
_Chapter VIII._—I have used chiefly _Wolf_ and _Delambre_; for the English writers Gascoigne and Horrocks I have used _Whewell_ and articles in the _Dict. Nat. Biog._ What I have said about the work of Huygens is taken directly from the books of his which are quoted in the text; and for special points I have consulted the _Principia_ of Descartes, and a very few of Cassini’s extensive writings.
There is no obvious book to recommend to students.
_Chapter IX._—For the external events of Newton’s life I have relied chiefly on Brewster’s _Memoirs of Sir Isaac Newton_; and for the history of the growth of his ideas on the subject of gravitation I have made extensive use of W. W. R. Ball’s _Essay on Newton’s Principia_, and of the original documents contained in it. I have also made some use of the articles on Newton in the _Encyclopaedia Britannica_ and the _Dictionary of National Biography_; as well as of Rigaud’s _Correspondence of Scientific Men of the Seventeenth Century_, of Edleston’s _Correspondence of Sir Isaac Newton and Prof. Cotes_, and of Baily’s _Account of the Rev^{d.} John Flamsteed_. The portrait is a reproduction of one by Kneller.
Students are recommended to read Brewster’s book, quoted above, or the abridged _Life of Sir Isaac Newton_ by the same author. The Laws of Motion are discussed in most modern textbooks of dynamics; the best treatment that I am acquainted with of the various difficulties connected with them is in an article by W. H. Macaulay in the _Bulletin of the American Mathematical Society_, Ser. II., Vol. III., No. 10, July 1897.
_Chapter X._—For Flamsteed I have used chiefly Baily’s _Account of the Rev^{d.} John Flamsteed_; for Bradley little but the _Miscellaneous Works and Correspondence of the Rev. James Bradley_ (edited by Rigaud), from which the portrait has been taken. My account of Halley’s work is based to a considerable extent on his own writings; there is a good deal of biographical information about him in the books already quoted in connection with Newton and Flamsteed, and there is a useful article on him in the _Dictionary of National Biography_. I have made a good deal of use in this chapter of _Wolf_ and _Delambre_, especially in dealing with Continental astronomers; and for special parts of the subject I have used Grant’s _History of Physical Astronomy_, Todhunter’s _History of the Mathematical Theories of Attraction and the Figure of the Earth_, and Poynting’s _Density of the Earth_.
_Chapter XI._—Most of the biographical material has been taken from _Wolf_ from articles in various encyclopaedias and biographical dictionaries, chiefly French, and from Delambre’s _Eloge_ of Lagrange. The two portraits are taken respectively from Serret’s edition of the _Oeuvres de Lagrange_ and from the Academy’s edition of the _Oeuvres Complètes de Laplace_. Gautier’s _Essai Historique sur le Problème des Trois Corps_ and Grant’s _History of Physical Astronomy_ have been the books most used for my account of the scientific contributions of the various astronomers dealt with; I have also consulted various modern treatises on gravitational astronomy, especially Tisserand’s _Mécanique Céleste_, Brown’s _Lunar Theory_, and to a less extent Cheyne’s _Planetary Theory_ and Airy’s _Gravitation_. For special points I have used Todhunter’s _History_, already referred to. Of the original writings I have made a good deal of use of Laplace’s _Mécanique Céleste_ as well as of his _Système du Monde_; I have also consulted a certain number of his other writings and of those of Lagrange and Clairaut; but have made no systematic study of them.
Students who wish to know more about gravitational astronomy but have little knowledge of mathematics should try to read Airy’s _Gravitation_; Herschel’s _Outlines of Astronomy_ and Grant’s _History_ (quoted above) also deal with the subject without employing mathematics, and are tolerably intelligible.
_Chapter XII._—The account of Herschel’s career is taken chiefly from Mrs. John Herschel’s _Memoir of Caroline Herschel_, from Miss A. M. Clerke’s _The Herschels and Modern Astronomy_, from the _Popular History of Astronomy in the Nineteenth Century_ by the same author, and from Holden’s _Sir William Herschel, his Life and Works_. The last three books and the _Synopsis and Subject Index to the Writings of Sir William Herschel_ by Holden & Hastings have been my chief guides to Herschel’s long series of papers; but nearly every thing that I have said about his chief pieces of work is based on his own writings. I have made also some little use of Grant’s _History_ (already quoted), of _Wolf_, and of Miss Clerke’s _System of the Stars_.
Students are recommended to read any or all of the first four books named above; the _Memoir_ gives a charming picture of Herschel’s personal life and especially of his relations with his sister. There is also a good critical account of Herschel’s work on sidereal astronomy in Proctor’s _Old and New Astronomy_.
_Chapter XIII._—Except in the articles dealing with gravitational astronomy I have constantly used Miss Clerke’s _History_ (already quoted), a book which students are strongly recommended to read; and in dealing with the first half of the century I have been helped a good deal by Grant’s _History_. But for the most part the materials for the chapter have been drawn from a great number of sources—consisting very largely of the original writings of the astronomers referred to—which it would be difficult and hardly worth while to enumerate; for the lives of astronomers (especially of English ones), as well as for recent astronomical history generally, I have been much helped by the obituary notices and the reports on the progress of astronomy which appear annually in the _Monthly Notices_ of the Royal Astronomical Society.
I add the names of a few books which deal with special parts of modern astronomy in a non-technical way:—
_The Sun_, C. A. Young; _The Sun_, R. A. Proctor; _The Story of the Sun_, R. S. Ball; _The Sun’s Place in Nature_, J. N. Lockyer.
_The Moon_, E. Neison; _The Moon_, T. G. Elger.
_Saturn and its System_, R. A. Proctor.
_Mars_, Percival Lowell.
_The World of Comets_, A. Guillemin (a well-illustrated but uncritical book, now rather out of date); _Remarkable Comets_, W. T. Lynn (a very small book full of useful information); _The Great Meteoritic Shower of November_, W. F. Denning.
_The Tides and Kindred Phenomena in the Solar System_, G. H. Darwin.
_Remarkable Eclipses_, W. T. Lynn (of the same character as his book on Comets.)
_The System of the Stars_, A. M. Clerke.
_Spectrum Analysis_, H. Schellen; _Spectrum Analysis_, H. E. Roscoe.
INDEX OF NAMES.
_Roman figures refer to the chapters, Arabic to the articles. The numbers given in brackets after the name of an astronomer are the dates of birth and death. All dates are_ A.D. _unless otherwise stated. In cases in which an authors name occurs in several articles, the numbers of the articles in which the principal account of him or of his work is given are printed in clarendon type thus_: =286=. _The names of living astronomers are italicised._
Abul Wafa. _See_ Wafa
Adams (1819-1892), XIII. 286, 287, 289
Adelard. _See_ Athelard
Airy (1801-1892), X. 227 _n_; XIII. =281=, =282=
Albategnius (?-929), II. 53; III. =59=, 66, 68 _n_; IV. 84, 85
Albert (of Prussia), V. 94
Albertus Magnus (13th cent.), III. 67
Alcuin (735-804), III. 65
Alembert, d’. _See_ D’Alembert
Alexander, II. 31
Alfonso X. (1223-1284), III. =66=, 68; V. 94
Al Mamun, III. 57, 69
Al Mansur, III. 56
Al Rasid, III. 56
Alva, VII. 135
Anaxagoras (499 B.C.?-427 B.C.?), I. 17
Anaximander (610 B.C.-546 B.C.?), I. 11
Apian (1495-1552), III. =69=; V. 97; VII. 146
Apollonius (latter half of 3rd cent. B.C.), II. =38=, 39, 45, 51,
52 _n_; X. 205
Arago, XII. 254
Archimedes, II. 52 _n_; III. 62
Argelander (1799-1875), XIII. 280
Aristarchus (earlier part of 3rd cent. B.C.), II. =24=, =32=, 41,
42, 54; IV. 75
Aristophanes, II. 19
Aristotle (384 B.C.-322 B.C.), II. 24, =27-30=, 31, 47, 51, 52;
III. 56, 66, 67, 68; IV. 70, 77; V. 100; VI. 116, 121, 125, 134;
VIII. 163
Aristyllus (earlier part of 3rd cent. B.C.), II. =32=, 42
Arzachel (_fl._ 1080), III. =61=, 66
d’Ascoli, Cecco (13th cent.), III. 67
Athelard (beginning of 12th cent.), III. 66
Auzout (?-1691), VIII. =155=, 160; X. 198
Bacon, Francis (1561-1627), VI. 134; VIII. 163
Bacon, Roger (1214?-1294), III. =67=; VI. 118
Bailly, XI. 237
_Ball_, XIII. 278 _n_
Bär, Reymers (Ursus) (?-1600), V. 105
Barberini (Urban VIII.), VI. 125, 127, 131, 132
_Barnard_, XIII. 294, 295
Baronius, VI. 125
Barrow, Isaac, IX. 166
Bayer, XII. 266
Bede, III. 65
Begh, Ulugh. _See_ Ulugh Begh
Bellarmine, VI. 126
Bentley, IX. 191
Berenice, I. 12
Bernouilli, Daniel (1700-1782), XI. 230
Bernouilli, James (1654-1705), XI. 230
Bernouilli, John (1667-1748), XI. 229, 230
Bessel (1784-1846), X. 198 _n_, 218; XIII. 272, =277-278=, 279, 280
Bille, V. 99
Bliss (1700-1764), X. 219
Bond, William Cranch (1789-1859), XIII. 295
Borelli (1608-1679), IX. 170
Bouguer (1698-1758), X. 219, =221=
Boullian. _See_ Bullialdus
Bouvard, XI. 247 _n_; XIII. 289
Bradley (1693-1762), X. 198, =206-218=, 219, 222-226; XI. 233;
XII. 257, 258, 263, 264; XIII. 272, 273, 275, 277
Brahe, Tycho (1546-1601), III. 60, 62; V. 97, 98 _n_, =99-112=;
VI. 113, 117, 127; VII. 136-139, 141 _n_, 142, 145, 146, 148;
VIII. 152, 153, 162; IX. 190; X. 198, 203, 225; XII. 257; XIII. 275
Brudzewski, IV. 71
Bruno, VI. 132
Bullialdus (1605-1694), XII. 266
Bunsen, XIII. 299
Burckhardt (1773-1825), XI. 241
Bürg (1766-1834), XI. 241
Bürgi (1552-1632), V. =97=, =98=; VIII. 157
Burney, Miss, XII. 260
_Burnham_, XIII. 309
Caccini, VI, 125
Caesar, II. 21; III. 67
Callippus (4th cent. B.C.), II. =20=, =26=, 27
Capella, Martianus (5th or 6th cent. A.D.), IV. 75
Carlyle, XI. 232
Carrington (1826-1875), XIII. 298, 302
Cartesius. _See_ Descartes
Cassini, Count (1748-1845), X. 220
Cassini, Giovanni Domenico (1625-1712), VIII. =160=, =161=; IX. 187;
X. 216, =220=, 221, 223; XII. 253, 267; XIII. 297
Cassini, Jacques (1677-1756), X. =220=, =221=, 222
Cassini de Thury (1714-1784), X. 220
Castelli, VI. 125
Catherine II., X. 227; XI. 230, 232
Cavendish (1731-1810), X. 219
Cecco d’Ascoli (1257?-1327), III. 67
_Chandler_, XIII. 285
Charlemagne, III. 65
Charles II., X. 197, 223
_Charlois_, XIII. 294
Christian (of Denmark), V. 106
Christine (the Grand Duchess), VI. 125
Clairaut (1713-1765), XI. 229, 230, =231=, 232, =233-235=, 237, 239,
248; XIII. 290
Clement VII., IV. 73
_Clerke_, XIII. 289 _n_
Clifford, IX. 173 _n_
Colombe, Ludovico delle, VI. 119 _n_
Columbus, III. 68
La Condamine (1701-1774), X. 219, =221=
Conti, VI. 125
Cook, X. 227
Coppernicus (1473-1543), II. 24, 41 _n_, 54; III. 55, 62, 69;
=IV.= _passim_; V. 93-97, 100, 105, 110, 111; VI. 117, 126, 127,
129; VII. 139, 150; IX. 186, 194; XII. 257; XIII. 279
_Cornu_, XIII. 283
Cosmo de Medici, VI. 121
Cotes (1682-1716), IX. 192
Crosthwait, X. 198
Cusa, Nicholas of (1401-1464), IV. 75
D’Alembert (1717-1783), X. 215; XI. 229, 230, 231 _n_, =232-235=,
237-239, 248
Damoiseau (1768-1846), XIII. 286
Dante, III. 67; VI. 119 _n_
_Darwin_, XIII. 292, 320
Da Vinci. _See_ Vinci
Dawes (1799-1868), XIII. 295
Delambre, II. 44; X. 218; XI. 247 _n_; XIII. 272
Delaunay (1816-1872), XIII 286, 287
De Morgan, II. 52 _n_
Descartes (1596-1650), VIII. 163
Diderot, XI. 232
Digges, Leonard (?-1571?), VI. 118
Digges, Thomas (?-1595), V. 95
Donati (1826-1873), XIII. 304
Doppler (1803-1853), XIII. 302
_Dreyer_, XIII. 308
_Dunér_, XIII. 302
Ecphantus (5th or 6th cent. B.C.), II. 24
Eddin, Nassir (1201-1273), III. =62=, 68; IV. 73
Encke (1791-1865), X. 227; XIII. 284
Eratosthenes (276 B.C.-195 or 196 B.C.), II. =33=, 45, 54; X. 221
Euclid (_fl._ 300 B.C.), II. 33, 52 _n_; III. 62, 66; VI. 115; IX. 165
Eudoxus (409 B.C.?-356 B.C.?), II. =26=, 27, 38, 42, 51
Euler (1707-1783), X. 215, 226; XI. 229, =230=, 231 _n_, =233-236=,
237, 239, 242, 243; XIII. 290
Fabricius, John (1587-1615?), VI. 124
Ferdinand (the Emperor), VII. 137, 147
Fernel (1497-1558), III. 69
Ferrel, XIII. 287
Field (1525?-1587), V. 95
Fizeau (1819-1896), XIII. 283
Flamsteed (1646-1720), IX. 192; X. =197=, =198=, 199, 204, 207 _n_,
218, 225; XII. 257; XIII. 275, 281
Fracastor (1483-1553), III. =69=; IV. 89; VII. 146
Fraunhofer (1787-1826), XIII. =299=, 311
Frederick II. (of Denmark), V. 101, 102, 106
Frederick II. (the Emperor), III. 66
Frederick II. (of Prussia), XI. 230, 232, 237
Galen, II. 20; III. 56; VI. 116
Galilei, Galileo (1564-1642), II. 30 _n_, 47; IV. 73; V. 96, 98 _n_;
=VI.= _passim_; VII. 135, 136, 138, 145, 151; VIII. 152-154, 157,
163; IX. 165, 168, 170, 171, 173, 179, 180, 186, 190, 195; X. 216;
XII. 253, 257, 263, 268; XIII. 278, 295
Galilei, Vincenzo, VI. 113
_Galle_, XIII. 281, 289
Gascoigne (1612?-1644), VIII. =155=, 156; X. 198
Gauss (1777-1855), XIII. =275=, =276=, 294
Gautier (1793-1881), XIII. 298
Genghis Khan, III. 62
George III, XII. 254-256
Gerbert (?-1003), III. 66
Gherardo of Cremona (1114-1187), III. 66
Gibbon, II. 53 _n_
Giese, IV. 74
Gilbert (1540-1603), VII. 150
_Gill_, XIII. 280, 281
_Glaisher_, XIII. 289 _n_
Godin (1704-1760), X. 221
Goodricke (1764-1786), XII. 266
Grant, XIII, 289 _n_
Grassi, VI. 127
Gregory, James (1638-1675), IX. =168=, 169; X. 202
Gregory XIII., II. 22
Gyldén (1841-1896), XIII. 288
Hainzel, V. 99
_Hale_, XIII. 301
Halifax, John. _See_ Sacrobosco
Halifax (Marquis of), IX. 191
_Hall_, XIII. 283 _n_, 295
Halley (1656-1742), VIII. 156; IX. =176=, =177=, 192 _n_; X. 198,
=199-205=, 206, 216, 223, 224, 227; XI. 231, 233, 235, 243;
XII. 265; XIII. 287, 290
Hansen (1795-1874), XIII. 282, 284, =286=, 290
_Harkness_, XIII. 301
Harriot (1560-1621), VI. 118, 124
Harrison, X. 226
Harun al Rasid, III. 56
Helmholtz (1821-1894), XIII. 319
Hencke (1793-1866), XIII. 294
Henderson (1798-1844), XIII. 279
Heraclitus (5th cent. B.C.), 11, 24
Herschel, Alexander, XII. 251
Herschel, Caroline (1750-1848), XII. 251, 254-256, 260
Herschel, John (1792-1871), I. 12; X. 221; XI. 242; XII. 256;
XIII. 289 _n_, =306-308=, 309, 316, 317, 319
Herschel, William (1738-1822), IX. 168; X. 223, 227; XI. 250;
=XII.= _passim_; XIII. 272, 273, 294, 296, 306-311, 317, 318
Hesiod, 11, 19, 20
Hevel (1611-1687), VIII. =153=; X. 198; XII. 268
Hicetas (6th or 5th cent. B.C.), II. 24; IV. 75
_Hill_, XI. 233 _n_; XIII. =286=, 290
Hipparchus (2nd cent. B.C.), I. 13; II. 25, 27, 31, 32, =37-44=,
45, 47-52, 54; III 63, 68; IV. 73, 84; V. 111; VII. 145
Hippocrates, III. 56
Holwarda (1618-1651), XII. 266
Holywood. _See_ Sacrobosco
Honein ben Ishak (?-873), III. 56
Hooke (1635-1703), IX. =174=, 176; X. 207, 212
Horky, VI. 121
Horrocks (1617?-1641), VIII. =156=; IX. 183; X. 204
_Howlett_, XIII. 298
_Huggins_, XIII. 301, 304, 311-313
Hulagu Khan, III. 62
Humboldt, XIII. 298
Hutton (1737-1823), X. 219
Huygens (1629-1695), V. 98 _n_; VI. 123; VIII. =154=, =155=, =157=,
=158=; IX. 170-172, 191
Hypatia (?-415), II. 53
Ibn Yunos. _See_ Yunos
Ishak ben Honein (?-910 or 911), III. 56
James I., V. 102; VII. 147
James II., IX. 192
_Janssen_, XIII. 301, 307 _n_
Joachim. _See_ Rheticus
Kaas, V. 106
Kant, XI. 250; XII. 258, 260; XIII. 287
_Kapteyn_, XIII. 280
_Kelvin_, XIII. 292
Kepler (1571-1630), II. 23, 51 _n_, 54; IV. 91; V. 94, 100, 104,
108-110; VI. 113, 121, 130, 132; =VII.= _passim_; VIII. 152, 156,
160; IX. 168-170, 172, 175, 176, 190, 194, 195; X. 202, 205, 220;
XI. 228, 244; XIII. 294, 301, 309
Kirchhoff (1824-1887), XIII. =299=, =300=, 311
Kirkwood (1815-1895), XIII. 294, 297
Koppernigk, IV. 71
Korra, Tabit ben. _See_ Tabit
Lacaille (1713-1762), X. =222-224=, 225, 227; XI. 230, 233, 235;
XII. 257, 259
La Condamine (1701-1774), X. 219, =221=
Lagrange (1736-1813), IX. 193; XI. 229, 231 _n_, 233 _n_, 236, =237=,
238-240, =242-245=, 247, 248; XII. 251; XIII. 293, 294
Lalande (1732-1807), XI. =235=, 241, 247 _n_; XII. 265
Lambert (1728-1777), XI. 243; XII. 265
Lami, IX. 180 _n_
Landgrave of Hesse. _See_ William IV.
_Langley_, XIII. 307
Lansberg (1561-1632), VIII. 156
Laplace (1749-1827), XI. 229, 231 _n_, =238-248=, =250=; XII. 251,
256; XIII. 272, 273, 282, 286-288, 290, 293, 297, 318-320
Lassell (1799-1880), XII. 267; XIII. =295=
Lavoisier, XI. 237
Legendre (1752-1833), XIII. =275=, 276
Leibniz, IX. 191, 193
Lemaire, XII. 255
Leverrier (1811-1877), XIII. 282, 284, =288=, =289=, 290, 293, 294
Lexell (1740-1784), XII. 253
Lindenau, XI. 247 _n_
Lionardo da Vinci. _See_ Vinci
Lippersheim (?-1619), VI. 118
Locke, IX. 191
_Lockyer_, XIII. 301, 302
_Loewy_, XIII. 283 _n_
Louis XIV., VIII. 160
Louis XVI., XI. 237
Louville (1671-1732), XI. 229
Lubbock (1803-1865), XIII. 286, 292
Luther, IV. 73; V. 93
Machin (?-1751), X. 214
Maclaurin (1698-1746), X. =196=; XI. 230, 231; XII. 251
Maestlin, VII. 135
Maraldi, X. 220
Marius (1570-1624), VI. =118=; VII. 145
Martianus Capella. _See_ Capella
Maskelyne (1732-1811), X. =219=; XII. 254, 265
Mason (1730-1787), X. 226; XI. 241
Matthias (the Emperor), VII. 143, 147
Maupertuis (1698-1759), X. 213, =221=; XI. 229, 231
Maxwell (1831-1879), XIII. 297
Mayer, Tobias (1723-1762), X. 217, =225=, =226=; XI. 233, 241;
XII. 265
Melanchthon, IV. 73, 74; V. 93
Messier (1730-1817), XII. 259, 260
Meton (460 B.C.?-?), II. 20
Michel Angelo, VI. 113
Michell, John (1724-1793), X. 219; XII. 263, 264
_Michelson_, XIII. 283
Molyneux (1689-1728), X. 207
Montanari (1632-1687), XII. 266
Müller. _See_ Regiomontanus
Napier, V. 97 _n_
Napoleon I., XI. 238; XII. 256
Napoleon, Lucien, XI. 238 _n_
Nassir Eddin. _See_ Eddin, Nassir
_Newcomb_, X. 227 _n_; XIII. =283=, =286=, 290
Newton (1643-1727). II. 54; IV. 75; VI. 130, 133, 134; VII. 144, 150;
VIII. 152; =IX.= _passim_; X. 196-200, 211, 213, 215-217, 219, 221;
XI. 228, 229, 231-235, 238, 249; XII. 257; XIII. 273, 299
Niccolini, VI. 132
Nicholas of Cusa (1401-1464), IV. 75
Nonius (1492-1577), III. 69
Norwood (1590?-1675), VIII. =159=; IX. 173
Numa, II. 21
Nunez. _See_ Nonius
_Nyrén_, XIII. 283 _n_
Olbers (1758-1840), XIII. 294
Orange, Prince of, V. 107
Osiander, IV. 74; V. 93
_Palisa_, XIII. 294
Palitzsch (1723-1788), XI. 231
Pemberton, IX. 192
Philolaus (5th cent. B.C.), II. =24=; IV. 75
Piazzi (1746-1826), XIII. 294
Picard (1620-1682), VIII. =155=, =157=, =159-161=, 162; IX. 174;
X. 196, 198, 221
_Pickering_, XIII. 314, 316
Plana (1781-1869), XIII. 286
Plato (428 B.C.?-347 B.C.?), II. =24=, =25=, 26, 51; IV. 70
Plato of Tivoli (_fl._ 1116), III. 66
Pliny (23 A.D.-79 A.D.), II. 45
Plutarch, II. 24; XIII. 301
Pogson (1829-1891), XIII. 316
_Poincaré_, XIII. 288
Poisson (1781-1840), XIII. 286, 293
Pontécoulant (1795-1874), XIII. 286
Porta, VI. 118
Posidonius (135 B.C.?-51 B.C.?), II 45, 47
Pouillet (1791-1868), XIII. 307, 319
Pound, X. 206, 216
Prévost (1751-1839), XII. 265
Pritchard (1808-1893), XIII. 278 _n_, =279=, 316
Ptolemy, Claudius (_fl._ 140 A.D.), II. 25, 27, 32, 37, =46-52=, 53,
54; III. 55, 57, 59-63, 68; IV. 70, 76, 80, 83-87, 89, 91; V. 94,
105; VI. 121, 129, 134; VII. 145; VIII. 161; IX. 194; X. 205;
XI. 236
Ptolemy Philadelphus, II. 31
Purbach (1423-1461), III. =68=; IV. 71
Pythagoras (6th cent. B.C.), I. 11, 14; II. =23=, 28, 47, 51, 54
Recorde (1510-1558), V. 95
Regiomontanus (1436-1476), III. =68=, 69; IV. 70, 71; V. 97, 110
Reimarus. _See_ Bär
Reinhold (1511-1553), V. =93-96=; VII. 139
Reymers. _See_ Bär
Rheticus (1514-1576), IV. =73=, =74=; V. =93=, =94=, 96
Ricardo, II. 47 _n_
Riccioli (1598-1671), VIII. 153
Richer (?-1696), VIII. =161=; IX. 180, 187; X. 199, 221
Rigaud. X. 206 _n_
Roemer (1644-1710), VIII. =162=; X. 198, 210, 216, 220, 225; XIII. 283
Rosse (1800-1867), XIII. 310, 317
Rothmann (_fl._ 1580), V. =97=, =98=, 106
Rudolph II. (the Emperor), V. 106-108; VII. 138, 142, 143
Sabine (1788-1883), XIII. 298
Sacrobosco (?-1256?), III. =67=, 68
St. Pierre, X. 197
Savary (1797-1841), XIII. 309
Scheiner (1575-1650), VI. =124=, 125; VII. =138=; VIII. =153=;
XII. 268
_Schiaparelli_, XIII. 297
Schomberg, IV. 73
Schoner, IV. 74
Schönfeld (1828-1891), XIII. 280
Schroeter (1745-1816), XII. 267, =271=
Schwabe (1789-1875), XIII. 298
Secchi (1818-1878), XIII. 311, 312
_See_, XIII. 320
Seleucus (2nd cent, B.C.), II. 24
Shakespeare, VI. 113
Sharp (1651-1742), X. 198
Slusius, IX. 169
Smith, XII. 251
Snell (1591-1626), VIII. 159; IX. 173
Sosigenes (_fl._ 45 B.C.), II. 21
South (1785-1867), XIII. 306
Struve, F. G. W. (1793-1864), XIII. 279, 309
_Struve, O._, XIII. 283 _n_
Svanberg (1771-1851), X. 221
Sylvester II. _See_ Gerbert
Tabit ben Korra (836-901), III. =56=, =58=, 68; IV. 84
Tamerlane, III. 63
_Tannery_, II. 36 _n_
Thales (640 B.C.?-546 B.C.?), II. =23=; III. 55
Theon (_fl._ 365 A.D.), II. 53
Theophrastus, II. 24
Theophylactus, IV. 72
Thomson, T., X. 208 _n_
_Thomson, William._ _See_ _Kelvin_
Thury, Cassini de. _See_ Cassini de Thury
Timocharis (beginning of 3rd cent. B.C.). II. =32=, 42; IV. 84
Tycho Brahe, _See_ Brahe
Ulugh Begh (1394-1449), III. =63=, 68; IV. 73
Urban VIII. (Barberini), VI. 125, 127, 131, 132
Ursus. _See_ Bär
Varignon, IX. 180 _n_
Vinci, Lionardo da (1452-1519), III. 69
_Vogel_, XIII. 313, 314
Voltaire, II. 21; XI, 229
Wafa, Abul (939 or 940-998), III. =60=, 68 _n_; IV. 85; V. 111
Wallenstein, VII. 149
Walther (1430-1504), III. 68; V. 97
Wargentin (1717-1783), X. 216
Watzelrode, IV. 71
Wefa. _See_ Wafa
Welser, VI. 124
Whewell (1794-1866), XIII. 292
William IV. (Landgrave of Hesse) (1532-1592), V. =97=, =98=, 100,
105, 106, 110
Wilson (1714-1786), XII. =268=; XIII. 298
_Wolf, Max_, XIII. 294
Wolf, Rudolf (1816-1893), XIII. 298
Wollaston (1766-1828), XIII. 299
Wren (1632-1723), IX. 174, 176
Wright, Thomas (1711-1786), XII. 258, 265
_Young_, XIII. 301
Yunos, Ibn (?-1008), III. =60=, 62, 68 _n_
von Zach, XI. 247 _n_
GENERAL INDEX.
_Roman figures refer to the chapters, Arabic to the articles. When several articles are given under one heading the numbers of the most important are printed in clarendon type, thus_: =207=. _The names of books are printed in italics._
Aberration, X. 206, =207-211=, 212, 213, 216, 218; XII. 263;
XIII. 277, 283, 284
Académie Française, XI. 232, 238
Academy of Berlin, XI. 230, 237
Academy of St. Petersburg, XI. 230, 233
Academy of Sciences (of Paris), X. 221, 223; XI. 229-233, 235-237
Academy of Turin, XI. 237, 238
Acceleration, VI. =133=; IX. =171=, 172, 173, 179, 180, 185, 195;
X. 223
_Ad Vitellionem Paralipomena_ (of Kepler), VII. 138
_Alae sive Scalae_ (of Digges), V. 95
Aldebaran, III. 64; XIII. 316 _n_
Alexandrine school, II. 21, 31-33, 36-38, 45, 53
_Alfonsine Tables_, III. =66=, 68; V. 94, 96, 99
Algol, XII. 266; XIII. 314, 315
_Almagest_ (of Ptolemy), II. =46-52=; III. 55, 56, 58, 60, 62, 66, 68;
IV. 75, 76, 83
_Almagest_ (of Abul Wafa), III. 60
_Almagest, New_ (of Kepler), VII. 148
_Almagest, New_ (of Riccioli), VIII. 153
_Almanac, Nautical_, X. 218; XIII. 286, 288, 290
Almanacks, I. 18 _n_; II. 20, 38; III. 64, 68; V. 94, 95, 100;
VII. 136; X. 218, 224; XIII. 286, 288, 290
Altair, III. 64; XIII. 316 _n_
Analysis, analytical methods, X. =196=; XI. 234
Angles, measurement of, I. 7
Annual equation, V. =111=; VII. 145
Annual motion of the earth. _See_ Earth, revolution of
Annual motion of the sun. _See_ Sun, motion of
Annual parallax. _See_ Parallax, stellar
Annular eclipse, II. =43=; VII. 145
Anomalistic month, II. 40
Ἀντιχθών, II. 24
Apex of solar motion, XII. 265
Aphelion, IV. 85
Apogee, II. =39=, 40, 48; III. 58, 59; IV. 85; V. 111; IX. 184 XI. 233
Apparent distance, I. 7
Apple, Newton’s, IX. 170
Apse, apse-line, II. =39=, 40, 48; IV. 85; IX. 183; XI. 235, 236, 242,
246
Arabic numerals, III. 64; V. 96
Arabs, Arab astronomy, II. 46, 53; III. =56-61=, =64=, 66, 68; V. 110;
VIII. 159; XII. 266
Arctic regions, II. 35
Arcturus, XII. 258
Aries, first point of (♈), I. =13=; II. 33, 42; IV. 83 _n_; V. 98,
III; X. 198
Asteroids. _See_ Minor planets
Astrolabe, II. 49; III. 66
Astrology, I. 16, =18=; III. 56; V. 99, 100; VII. 136, 149, 151
_Astronomiae Fundamenta_ (of Lacaille), X. 224
_Astronomiae Instauratae Mechanica_ (of Tycho), V. 107
_Astronomiae Instauratae Progvmnasmata_ (of Tycho), V. 104
Astronomical Society, German, XIII. 280
Astronomical Society, Royal, XII. 256, 263
_Astronomicum Caesareum_ (of Apian), V. 97
_Astronomisches Jahrbuch_, XII. 253
Astronomy, divisions of, XIII. 272
Astronomy, descriptive, XIII. =272=, 273, 294
Astronomy, gravitational, X. =196=; XIII. 272, 273, 286
Astronomy, observational, XIII. 272, 273
Astronomy, origin of, I. =2=
Astronomy, scope of, I. 1
Attraction. _See_ Gravitation
Autumnal equinox, I. II. _See also_ Equinox
Axioms. _See_ Laws of Motion
Axis (of an ellipse), XI. 236, 244, 245
Babylonians. _See_ Chaldaeans
Bagdad, III. 56, 57, 60, 68
Belts of Jupiter, XII. 267
Betelgeux, III. 64
Biela’s comet, XIII. 305
Binary stars. _See_ Stars, double and multiple
Bode’s _Astronomisches Jahrbuch_, XII. 253
Bodily tides, XIII. 292, 293
Brightness of stars. _See_ Stars, brightness of
Brooks’s comet, XIII. 305
Brucia, XIII. 294
Bureau des Longitudes, XI. 238
Cairo, III. 60
Calculus of Variations, XI. 237 _n_
Calendar, Greek, II. =19=, =20=, 21
Calendar, Gregorian, II. =22=; IX. 165 _n_; X. 217
Calendar, Julian, II. =21=, 22; III. 68; IV. 73; IX. 165 _n_;
X. 197 _n_, 217
Calendar, Mahometan, III. 56
Calendar, Roman, II. 21
Caliphs, III. 56, 57, 69
Canals of Mars, XIII. 297
Cartesianism, VIII. 163; IX. 191, 195; XI. 229
Castor, XII. 263, 264, 266
Catalogues of stars. _See_ Star-catalogues
Cavendish experiment, X. 219
Celestial latitude. _See_ Latitude, celestial
Celestial longitude. _See_ Longitude, celestial
Celestial sphere, I. =7=, =8=, 9-11, 13, 14; II. 24, 26, 33, 38-40,
45, 47, 51; III. 64, 67; IV. 78, 80, 83, 88; V. 98, 105; VI. 129;
VIII. 157; X. 198, 207, 208, 214; XII. 257; XIII. 272
Celestial sphere, daily motion of. _See_ Daily motion
Celestial spheres, II. 23, 26, 27, 38, 51, 54; III. 62, =68=; V. 100,
103
Centre of gravity, IX. 186
Centrifugal force, VIII. 158 _n_
Ceres, XIII. 276, 294
Chaldaeans (Babylonians), Chaldaean astronomy, I. 6, 11, 12, =16-18=;
II. 30, 34, 40, 51, 54; III. 56
Chart, photographic, XIII. 280
Chemistry of the sun, XIII. =299-301=, 303
Chinese astronomy, I. 6, 11
Chords, II. 47 _n_
Chromosphere, X. 205; XIII. =301=, 303
Chronometer, X. 226
Circular motion, II. 25, 26, 38, 51; IV. 76; VII. 139; VIII. =158=;
IX. =171-173=. _See also_ Eccentric, Epicycle
Circumpolar stars, I. =9=; II. 35
Clock. _See_ Pendulum clock _and_ Chronometer
Clustering power, XII. 261. _See also_ Condensation of nebulae
_Coelum Australe Stelliferum_ (of Lacaille), X. 223
Collimation error, X. 225 _n_
Comets, I. 1; II. 30; III. 68, =69=; V. 100, 103-105; VI. 127, 129;
VII. 144, =146=; VIII. 153; IX. =190=, 192; X. =200=, 205, 217,
224; XI. 228, =231=, 243, 248, 250; XII. 253, 256, 259;
XIII. 272, =291=, =304=, =305=, 307
Comet, Biela’s, XIII. 305
Comet, Brooks’s, XIII. 305
Comet, Encke’s, XIII. 291
Comet, Halley’s, VII. 146; X. =200=, 205; XI. =231=, 232; XIII. 291,
307
Comet, Lexell’s, XI. 248; XIII. 305
Comet, Olbers’s, XIII. 291
Comet, Pons-Brooks, XIII. 291
Comet, Tebbutt’s, XIII. 305
Comet, Tuttle’s, XIII. 291
_Cometographia_ (of Hevel), VIII. 153
_Commentaries on the Motions of Mars_ (of Kepler), VII. 135 _n_,
139, 141, 150 _n_
_Commentariolus_ (of Coppernicus), IV. =37=; V. 100
_Compleat System of Optics_ (of Smith), XII. 251
Complete induction, IX. 195
Condensation of nebulae, XI. 250; XII. 261; XIII. 318
Conic, conic section, VII. =140= _n_; XIII. 309
Conjunction, II. =43=, 48 _n_; III. 60; V. 110, III; X. 227
Conservation of energy, XIII. 319
Constant of aberration, X. =209=, 210; XIII. 283 _n_
Constellations, I. =12=, 13; II. 20, =26=, 34, =42=; X. =223=
Construction of the heavens, XII. 257. _See also_ Sidereal system,
structure of
Corona, VII. 145; X. 205; XIII. =301=, 303
Counter-earth, II. 24
Crape-ring, XII. 267; XIII. 295
Craters (on the moon), VIII. 153; XIII. 296
Curvature of the earth. _See_ Earth, shape of
Daily Motion (of the celestial sphere), I. 5, =8=, =9=, 10; II. 23,
24, 26, 33, 38, 39, 46, 47; III. 67, 68; IV. =78=, =80=, 83;
V. 98, 105; VI. 129; VIII. 157
D’Alembert’s principle, XI. 232, 237 _n_
Damascus, III. 57
_Darlegung_ (of Hansen), XIII. 286
Day, I. 4, II. 16; II. 47; XIII. 287, 293, 320
Day-and-night, I. 16 _n_
Day-hour, I. 16
Declination, II. =33=, 35, 39; X. 213, 218; XIII. 276
Declination circle, II. 33
_De Coelo_ (of Aristotle), II. 27
Deductive method, inverse, IX. 195
Deferent, II. =39=, 48, 51; III. 68; IV. 86, 87
Degree, I. 7
Deimos, XIII. 295
_De Magnete_ (of Gilbert), VII. 150
_De Motu_ (of Newton), IX. 177, 191
_De Mundi aetherei_ (of Tycho), V. 104
_De Nova Stella_ (of Tycho), V. 100
_De Revolutionibus_ (of Coppernicus), II. 41 _n_; IV. =74-92=;
V. 93, 94; VI. 126
_De Saturni Luna_ (of Huygens), VIII. 154
Descriptive astronomy, XIII. =272=, 273, 294
Deviation error, X. 225 _n_
_Dialogue on the Two Chief Systems_ (of Galilei), VI. 124 _n_,
=128-132=, 133
Differential method of parallax, VI. =129=; XII. 263; XIII. 278
Diffraction-grating, XIII. 299
Dione, VIII. 160
_Dioptrice_ (of Kepler), VII. 138
Direct motion, I. 14
Disturbing force. _See_ Perturbations
Diurnal method of parallax, XIII. =281=, 284
Doctrine of the sphere. _See_ Spherics
Doppler’s principle, XIII. =302=, 313, 314
Double hour, I. 16
Double-star method of parallax. _See_ Differential method of parallax
Double stars. _See_ Stars, double and multiple
Draconitic month, II. =40=, 43
_Durchmusterung_, XIII. 280
Dynamics, VI. 133, 134; IX. 179, 180; XI. 230, 232, 237
_Dynamique, Traité de_ (of D’Alembert), XI. 232
Earth, I. 1, 15, 17; II. 28, 29, 32, 39, 41, 43, 47, 49, 51; III. 66,
69; IV. 80, 86; VI. 117, 121, 133; VII. 136 _n_, 144, 145, 150;
VIII. 153, 154; IX. 173, 174, 179-182, 184, 186, 195; XI. 228, 245;
XIII. 285, 287, 292, 293, 297, 320. _See also_ the following
headings
Earth, density, mass of, IX. 180, 185, 189; X. =219=; XI. 235;
XIII. 282, 294
Earth, motion of, II. 24, 32, 47; IV. =73=, 76, =77=; V. 96. 97,
=105=; VI. 121, 125-127, =129-132=; VIII. 161, 162; IX. 186, 194;
XII. 257. _See also_ Earth, revolution of _and_ rotation of
Earth, revolution of, annual motion of, II. 23, =24=, 28 _n_, =30=,
47; IV. =75=, =77=, =79-82=, =85-88=, 89, 90, =92=; V. 111;
VI. 119, 126, =129=, 131, 133; VII. 139, 142, 146; VIII. 161;
IX. 172, 183; X. 207-210, 212, 227; XI. 235, 236, 240; XII. 263;
XIII. 278, 282, 283
Earth, rigidity of, XIII. 285, 292
Earth, rotation of, daily motion of, II. 23, =24=, 28 _n_; IV. =75=,
=78=, 79 _n_, =80=, 84; V. =105=; VI. 124, 126, =129=, =130=;
IX. 174, 194; X. 206, 207, 213; XIII. 281, 285, =287=, 320
Earth, shape of, II. =23=, =29=, =35=, =45=, =47=, 54; IV. 76; VIII.
=161=; IX. =187=, 188; X. 196, 213, 215, 220, =221=, 222, 223; XI.
229, =231=, 237, 248
Earth, size of, II. =36=, 41, 45, 47, 49; III. 57, 69; IV. 85;
VII. 145; VIII. =159=, 161; IX. 173, 174; X. =221=, 222, 223
Earth, zones of, II. =35=, 47
Earthshine, III. 69
Easter, rule for fixing, II. 20
Eccentric, II. 37, =39=, =40=, 41, =48=, =51=; III. 59; IV. =85=, =89=,
=91=; VII. 139, 150
Eccentricity, II. =39=; IV. 85; VII. =140= _n_; XI. 228, 236, 240,
244-246, 250; XIII. 294, 318
Eccentricity fund, XI. 245
Eclipses, I. 11, 15, =17=; II. 29, 32, 40-42, =43=, 47-49, 54;
III. 57, 68; IV. 76, 85; V. 110; VI. 127; VII. 145, 148: VIII. 162;
X. 201, 205, 210, 216, 227; XI. 240; XIII. 287, 301
Eclipses, annular, II. =43=; VII. 145
Eclipses, partial, II. 43
Eclipses, total, II. =43=; VII. 145; X. 205; XIII. =301=
Ecliptic, I. =11=, 13, 14; II. 26, 33, 35, 36, 38, 40, 42, 51; III.
58, 59, 68; IV. 80, 82-84, 87, 89; V. 111; VIII. 154; X. 203, 209,
213, 214, 227; XI. 235, 236, 244, 246, 250
Ecliptic, obliquity of, I. =11=; II. 35, 36, 42; III. 59, 68; IV. 83,
84; XI. 235, 236
École Normale, XI. 237, 238
École Polytechnique, XI. 237
Egyptians, Egyptian astronomy, I. 6, 11, 12, 16; II. 23, 26, 30, 45;
IV. 75
_Elements_ (of Euclid), III. 62, 66; IX. 165
Elements (of an orbit), XI. =236=, 240, 242, 244, 246; XIII. 275, 276
Elements, variation of. _See_ Variation of elements
Ellipse, II. 51 _n_; III. 66; VII. =140=, 141; IX. 175, 176, 190, 194;
X. 200, 209, 214; XI. 228, 236, 242, 244; XIII. 276, 278, 309
Ellipticity, X. 221
Empty month, II. =19=, 20
Empyrean, III. 68
Enceladus, XII. 255
Encke’s comet, XIII. 291
Encyclopaedia, the French, XI. 232
Energy, XIII. 319
Ephemerides. _See_ Almanacks
_Ephemerides_ (of Regiomontanus), III. 68
Epicycle, II. 37, =39=, 41, 45, =48=, =51=, 54; III. 68; IV. =85-87=,
=89-91=; VII. 139, 150; VIII. 163; IX. 170, 194
_Epitome_ (of Kepler), VI. 132; VII. 144, =145=
_Epitome_ (of Purbach), III. 68
Equant, II. =51=; III. 62; IV. 85, 89, 91; VII. 139, 150
Equation of the centre, II. =39=, 48; III. 60; V. 111
Equator, I. =9=, 10, 11; II. 33, 35, 39, 42; IV. 82, 84; V. 98;
VI. 129, 133; IX. 187; X. 207, 220, 221; XIII. 285
Equator, motion of. _See_ Precession
Equinoctial points, I. =11=, 13; II. 42. _See also_ Aries, first
point of
Equinoxes, I. =11=; II. 39, 42
Equinoxes, precession of. _See_ Precession
_Essai philosophique_ (of Laplace), XI. 238
Ether, XIII. 293, 299
Evection, II. =48=, 52; III. 60; IV. 85; V. 111; VII. 145
Evening star, I. 14. _See also_ Venus
_Exposition du Système du Monde_ (of Laplace), XI. =238=, 242 _n_,
=250=
Faculae, VIII. =153=; XIII. 300, 301, 303
Figure of the earth. _See_ Earth, shape of
Firmament, III. 68
First point of Aries, Libra. _See_ Aries, Libra, first point of
Fixed stars, I. 14. _See_ Stars
Fluxions, IX. 169, 191; X. 196
_Fluxions_ (of Maclaurin), XII. 251
Focus, VII. =140=, 141; IX. 175; XI. 236
Force, VI. 130; IX. =180=, 181
Fraunhofer lines, XIII. =299=, =300=, 303, 304
Front-view construction. _See_ Herschelian telescopes
Full month, II. =19=, 20
Full moon. _See_ Moon, phases of
_Fundamenta_ (of Hansen), XIII. 286
_Fundamenta Astronomiae_ (of Bessel), X. 218; XIII. =277=
Funds of eccentricity, inclination, XI. 245
Galactic circle, XII. 258, 260
Galaxy. _See_ Milky Way
Gauges, gauging. _See_ Star-gauging
Georgium Sidus. _See_ Uranus
Gravitation, gravity, II. 38 _n_; VII. 150; VIII. 158, 161;
=IX.= _passim_; X. 196, 201, 213, 215, 219, 220, 223, 226;
=XI.= _passim_; XII. 264; XIII. 282, 284, 286-293, 309, 319
Gravitational astronomy, X. =196=; XIII. 272, 273, 286
Gravity, variation of, VIII. =161=; IX. 180; X. 199, 217, 221, 223;
XI. =231=
Great Bear, I. 12; XII. 266
Great circle, I. =11=; II. 33, 42; IV. 82, 84
Gregorian Calendar. _See_ Calendar, Gregorian
Grindstone theory, XII. =258=; XIII. 317
_Hakemite Tables_, III. =60=, 62
Halley’s comet, VII. 146; X. =200=, 205; XI. =231=, 232; XIII. 291, 307
_Harmonics_ (of Smith), XII. 251
_Harmony of the World_ (of Kepler), VII. 144
Helium, XIII. 301
Herschelian telescope, XII. 255, 256
_Historia Coelestis_ (of Flamsteed), X. 198
Holy Office. _See_ Inquisition
Horizon, I. 3, 9; II. 29, =33=, 35, 39, 46; VIII. 161; XIII. 285
Horoscopes, V. 99
Hour, I. 16
Hydrostatic balance, VI. 115 _n_
Hyperbola, IX. 190; XI. 236 _n_
Hyperion, XIII. 295
_Ilkhanic Tables_, III. 62
_Il Saggiatore_ (of Galilei), VI. 127
Inclination, III. 58; IV. 89; XI. =228=, =244=, 245, 246, 250;
XIII. 294, 318
Inclination fund, XI. 245
_Index of Prohibited Books_, VI. 126, 132; VII. 145
Indians, Indian astronomy, I. 6; III. 56, 64
Induction, complete, IX. 195
Inequalities, long, XI. 243
Inequalities, periodic, XI. =242=, 243, 245, 247
Inequalities, secular, XI. =242=, 243-247; XIII. 282. _See also_
Perturbations
Inequality, parallactic, XIII. 282
Inferior planets, I. =15=; IV. 87, 88. _See also_ Mercury, Venus
Inquisition (Holy Office), VI. 126, 132, 133
Institute of France, XI. 241
Inverse deductive method, IX. 195
Inverse square, law of, IX. =172-176=, =181=, 195; XI. 233. _See also_
Gravitation
Ionian school, II. 23
Iris, XIII. 281
Irradiation, VI. 129
Island universe theory, XII. =260=; XIII. 317
Japetus, VIII. 160; XII. 267; XIII. 297
Julian Calendar. _See_ Calendar, Julian
Juno, XIII. 294
Jupiter, I. 14-16; 11. 25, 51; IV. 81, 87, 88; V. 98, 99; VI. 121,
127; VII. 136 n, 142, 144, 145, 150; VIII. 154, 156, 162; IX. 172,
181, 183, 185-187; X. 204, 216; XI. 228, 231, 235, 236, 243-245,
248; XII. =267=; XIII. 281, 288, 294, =297=, 305. _See also_ the
following headings
Jupiter, belts of, XII. 267
Jupiter, mass of, IX. 183, 185
Jupiter, rotation of, VIII. =160=; IX. 187; XIII. =297=
Jupiter, satellites of, II. 43; VI. =121=, =127=, 129, 133; VII.
=145=, 150; VIII. 160, 162; IX. 170, 184, 185; X. 210, =216=;
XI. 228, =248=; XII. 267; XIII. 283, =295=, 297
Jupiter’s satellites, mass of, XI. 248
Kepler’s Laws, VII. =141=, =144=, 145, 151; VIII. 152; IX. 169, 172,
175, 176, 186, 194, 195; X. 220; XI. 244; XIII. 294, 309
Latitude (celestial), II. =33=, 42, 43; III. 63; IV. 89
Latitude (terrestrial), III. 68, 69; IV. 73; X. =221=; XIII. 285
Latitude, variation of, XIII. 285
Law of gravitation. _See_ Gravitation
Laws of motion, VI. =130=, =133=; VIII. 152, 163; IX. 171, =179-181=,
183, 186, 194, 195; XI. 232
Leap-year, I. 17; II. =21=, 22
Least squares, XIII. =275=, 276
_Letter to the Grand Duchess_ (of Galilei), VI. 125
Level error, X. 225 _n_
Lexell’s comet, XI. 248; XIII. 305
Libra, first point of (♎), I. =13=; II. 42
Librations of the moon, VI. =133=; X. 226; XI. =237=, 239
_Libros del Saber_, III. 66
Light-equation, XIII. 283
Light, motion of, velocity of, VIII. =162=; X. 208-211, 216, 220;
XIII. 278, 279, =283=, 302. _See also_ Aberration
Logarithms, V. 96, 97 _n_
Long inequalities, XI. 243
Longitude (celestial), II. =33=, 39, 42, 43; III. 63; IV. 87; VII. 139
Longitude (terrestrial), III. 68; VI. =127=, 133; VII. 150; X. 197,
216, =226=
Longitudes, Bureau des, XI. 238
Lunar distances, III. 68 _n_
Lunar eclipses. _See_ Eclipses
Lunar equation, XIII. 282
Lunar theory, II. =48=, 51; V. 111; VII. 145; VIII. 156; IX. =184=,
192; X. =226=; XI. =228=, 230, 231, =233=, =234=, =240=, =241=,
242, 248; XIII. 282, =286=, =287=, 288, 290. _See also_ Moon,
motion of
Lunation, II. =40=. _See also_ Month, synodic
_Macchie Solari_ (of Galilei), VI. =124=, 125
Magellanic clouds, XIII. 307
Magnetism, VII. 150; XIII. 276, =298=
_Magnitudes and Distances of the Sun and Moon_ (of Aristarchus), II. 32
Magnitudes of stars, II. 42; XII. 266; XII. 280, 316. _See also_
Stars, brightness of
Mars, I. 14-16; II. 25, 26, 30, 51; III. 68; IV. 81, 87; V. 108; VI.
129; VII. 136 _n_, 139-142, 144, 145; VIII. 154, 161; IX. 181, 183,
185; X. 223, 227; XI. 235, 245; XII. 267; XIII. 281, 282, 284, 294,
295, =297=. _See also_ the following headings
Mars, canals of, XIII. 297
Mars, mass of, XI. 248
Mars, opposition of, VIII. =161=; XIII. =281=, 284, 297
Mars, rotation of, VIII. 160; XIII. 295, 297
Mars, satellites of, XIII. 295
Mass, IX. =180=, 181, 185
Mass of the earth, sun, Venus.... _See_ Earth, Sun, Venus ... mass of
_Mécanique Analytique_ (of Lagrange), XI. 237
_Mécanique Celeste_ (of Laplace), XI. =238=, 241, 247, 249, 250;
XIII. 292
Medicean Planets. _See_ Jupiter, satellites of
Meraga, III. 62
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A Short History of AstronomyChapter XIII: The Nineteenth Century (3)
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