CONTENTS.

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Preface v
CHAPTER I.
Primitive Astronomy, §§1-18 1-20
§1. Scope of astronomy 1
§§2-5. First notions: the motion of the sun: the motion and phases of the moon: daily motion of the stars 1
§6. Progress due to early civilised peoples: Egyptians, Chinese, Indians, and Chaldaeans 3
§7. The celestial sphere: its scientific value: apparent distance between the stars: the measurement of angles 4
§§8-9. The rotation of the celestial sphere: the North and South poles: the daily motion: the celestial equator: circumpolar stars 7
§§10-11. The annual motion of the sun: great circles: the ecliptic and its obliquity: the equinoxes and equinoctial points: the solstices and solstitial points 8
§§12-13. The constellations: the zodiac, signs of the zodiac, and zodiacal constellations: the first point of Aries (?), and the first point of Libra (?) 12
§14. The five planets: direct and retrograde motions: stationary points 14
§15. The order of nearness of the planets: occultations: superior and inferior planets 15
§16. Measurement of time: the day and its division into hours: the lunar month: the year: the week 17
§17. Eclipses: the saros 19
§18. The rise of Astrology 20
CHAPTER II.
Greek Astronomy (from about 600 b.c. to about 400 a.d.), §§19-54 21-75
§§19-20. Astronomy up to the time of Aristotle. The Greek calendar: full and empty months: the octaeteris: Meton’s cycle 21
§21. The Roman calendar: introduction of the Julian Calendar 22
§22. The Gregorian Calendar 23
§23. Early Greek speculative astronomy: Thales and Pythagoras: the spherical form of the earth: the celestial spheres: the music of the spheres 24
§24. Philolaus and other Pythagoreans: early believers in the motion of the earth: Aristarchus and Seleucus 25
§25. Plato: uniform circular and spherical motions 26
§26. Eudoxus: representation of the celestial motions by combinations of spheres: description of the constellations. Callippus 27
§§27-30. Aristotle: his spheres: the phases of the moon: proofs that the earth is spherical: his arguments against the motion of the earth: relative distances of the celestial bodies: other speculations: estimate of his astronomical work 29
§§31-2. The early Alexandrine school: its rise: Aristarchus: his estimates of the distances of the sun and moon. Observations by Timocharis and Aristyllus 34
§§33-4. Development of spherics: the Phenomena of Euclid: the horizon, the zenith, poles of a great circle, verticals, declination circles, the meridian, celestial latitude and longitude, right ascension and declination. Sun-dials 36
§35. The division of the surface of the earth into zones 37
§119. The Sidereus Nuncius: observations of the moon 150
§120. New stars: resolution of portions of the Milky Way 151
§121. The discovery of Jupiter’s satellites: their importance for the Coppernican controversy: controversies 151
§122. Appointment at the Tuscan court 153
§123. Observations of Saturn. Discovery of the phases of Venus 154
§124. Observations of sun-spots by Fabricius, Harriot, Scheiner, and Galilei: the Macchie Solari: proof that the spots were not planets: observations of the umbra and penumbra 154
§125. Quarrel with Scheiner and the Jesuits: theological controversies: Letter to the Grand Duchess Christine 157
§126. Visit to Rome. The first condemnation: prohibition of Coppernican books 159
§127. Method for finding longitude. Controversy on comets: Il Saggiatore 160
§128. Dialogue on the Two Chief Systems of the World. Its preparation and publication 162
§129. The speakers: argument for the Coppernican system based on the telescopic discoveries: discussion of stellar parallax: the differential method of parallax 163
§130. Dynamical arguments in favour of the motion of the earth: the First Law of Motion. The tides 165
§131. The trial and condemnation. The thinly veiled Coppernicanism of the Dialogue: the remarkable preface 168
§132. Summons to Rome: trial by the Inquisition: condemnation, abjuration, and punishment: prohibition of the Dialogue 169
§133. Last years: life at Arcetri: libration of the moon: the Two New Sciences: uniform acceleration, and the first law of motion. Blindness and death 172
§134. Estimate of Galilei’s work: his scientific method 176
CHAPTER VII.
Kepler (from 1571 a.d. to 1630 a.d.), §§135-151 179-197
§135. Early life and theological studies 179
§136. Lectureship on mathematics at Gratz: astronomical studies and speculations: the Mysterium Cosmographicum 180
§137. Religious troubles in Styria: work with Tycho 181
§138. Appointment by the Emperor Rudolph as successor to Tycho: writings on the new star of 1604 and on Optics: theory of refraction and a new form of telescope 182
§139. Study of the motion of Mars: unsuccessful attempts to explain it 183
§§140-1. The ellipse: discovery of the first two of Kepler’s Laws for the case of Mars: the Commentaries on Mars 184
§142. Suggested extension of Kepler’s Laws to the other planets 186
§143. Abdication and death of Rudolph: appointment at Linz 188
§144. The Harmony of the World: discovery of Kepler’s Third Law: the “music of the spheres” 188
§145. Epitome of the Copernican Astronomy: its prohibition: fanciful correction of the distance of the sun: observation of the sun’s corona 191
§146. Treatise on Comets 193
§147. Religious troubles at Linz: removal to Ulm 194
§238. Laplace: his career: the MÉcanique CÉleste and the SystÈme du Monde: political appointments and distinctions 306
§239. Advance made by Lagrange and Laplace on the work of their immediate predecessors 308
§240. Explanation of the moon’s secular acceleration by Laplace 308
§241. Laplace’s lunar theory: tables of BÜrg and Burckhardt 309
§242. Periodic and secular inequalities 310
§243. Explanation of the mutual perturbation of Jupiter and Saturn: long inequalities 312
§§244-5. Theorems on the stability of the solar system: the eccentricity fund and the inclination fund 313
§246. The magnitudes of some of the secular inequalities 318
§247. Periodical inequalities: solar and planetary tables MÉcanique CÉleste 318
§248. Minor problems of gravitational astronomy: the satellites: Saturn’s ring: precession and nutation: figure of the earth: tides: comets: masses of planets and satellites 318
§249. The solution of Newton’s problem by the astronomers of the eighteenth century 319
§250. The nebular hypothesis: its speculative character 320
CHAPTER XII.
Herschel (from 1738 a.d. to 1822 a.d.), §§251-271 323-353
§§251-2. William Herschel’s early career: Bath: his first telescope 323
§§253-4. The discovery of the planet Uranus, and its consequences: Herschel’s removal to Slough 325
§255. Telescope-making: marriage: the forty-foot telescope: discoveries of satellites of Saturn and of Uranus 327
§256. Life and work at Slough: last years: Caroline Herschel 328
§257. Herschel’s astronomical programme: the study of the fixed stars 330
§258. The distribution of the stars in space: star-gauging: the “grindstone” theory of the universe: defects of the fundamental assumption: its partial withdrawal. Employment of brightness as a test of nearness: measurement of brightness: “space-penetrating” power of a telescope 332
§259. Nebulae and star clusters: Herschel’s great catalogues 336
§260. Relation of nebulae to star clusters: the “island universe” theory of nebulae: the “shining fluid” theory: distribution of nebulae 337
§261. Condensation of nebulae into clusters and stars 339
§262. The irresolvability of the Milky Way 340
§263. Double stars: their proposed employment for finding parallax: catalogues: probable connection between members of a pair 341
§264. Discoveries of the revolution of double stars: binary stars: their uselessness for parallax 343
§265. The motion of the sun in space: the various positions suggested for the apex 344
§266. Variable stars: Mira and Algol: catalogues of comparative brightness: method of sequences: variability of ? Herculis 346
§267. Herschel’s work on the solar system: new satellites: observations of Saturn, Jupiter, Venus, and Mars 34

                                                                                                                                                                                                                                                                                                           

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