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THESTORYOFTHEHEAVENS
PLATE I.
THE PLANET SATURN,
IN 1872.
THE
Story oftheHeavens
SIR ROBERT STAWELL BALL, LL.D. D.Sc.
Author of "Star-Land"
FELLOW OFTHE ROYAL SOCIETY OF LONDON, HONORARY FELLOW OF
THE ROYAL SOCIETY OF
EDINBURGH, FELLOW OFTHE ROYAL ASTRONOMICAL SOCIETY,
SCIENTIFIC ADVISER TO THE
COMMISSIONERS OF IRISH LIGHTS, LOWNDEAN PROFESSOR OF
ASTRONOMY AND
GEOMETRY IN THE UNIVERSITY OF CAMBRIDGE, AND FORMERLY
ROYAL ASTRONOMER OF IRELAND
WITH TWENTY-FOUR COLOURED PLATES AND NUMEROUS
ILLUSTRATIONS
NEW AND REVISED EDITION
CASSELL and COMPANY, Limited
LONDON, PARIS, NEW YORK & MELBOURNE
1900
ALL RIGHTS RESERVED
PREFACE TO ORIGINAL EDITION.
I have to acknowledge the kind aid which I have received in the preparation of this
book.
Mr. Nasmyth has permitted me to use some ofthe beautiful drawings ofthe Moon,
which have appeared in the well-known work published by him in conjunction with
Mr. Carpenter. To this source I am indebted for Plates VII., VIII., IX., X., and Figs.
28, 29, 30.
Professor Pickering has allowed me to copy some ofthe drawings made at Harvard
College Observatory by Mr. Trouvelot, and I have availed myself of his kindness for
Plates I., IV., XII., XV.
I am indebted to Professor Langley for Plate II., to Mr. De la Rue for Plates III. and
XIV., to Mr. T.E. Key for Plate XVII., to Professor Schiaparelli for Plate XVIII., to
the late Professor C. Piazzi Smyth for Fig. 100, to Mr. Chambers for Fig. 7, which has
been borrowed from his "Handbook of Descriptive Astronomy," to Dr. Stoney for Fig.
78, and to Dr. Copeland and Dr. Dreyer for Fig. 72. I have to acknowledge the
valuable assistance derived from Professor Newcomb's "Popular Astronomy," and
Professor Young's "Sun." In revising the volume I have had the kind aid ofthe Rev.
Maxwell Close.
I have also to thank Dr. Copeland and Mr. Steele for their kindness in reading through
the entire proofs; while I have also occasionally availed myself ofthe help of Mr.
Cathcart.
ROBERT S. BALL.
Observatory, Dunsink, Co. Dublin.
12th May, 1886.
NOTE TO THIS EDITION.
I have taken the opportunity in the present edition to revise the work in accordance
with the recent progress of astronomy. I am indebted to the Royal Astronomical
Society for the permission to reproduce some photographs from their published series,
and to Mr. Henry F. Griffiths, for beautiful drawings of Jupiter, from which Plate XI.
was prepared.
ROBERT S. BALL.
Cambridge,
1st May, 1900.
CONTENTS.
page
Introduction 1
chapter
I.
The Astronomical
Observatory
9
II. The Sun 29
III. The Moon 70
IV. The Solar System 107
V. The Law of Gravitation 122
VI. The Planet of Romance 150
VII. Mercury 155
VIII. Venus 167
IX. The Earth 192
X. Mars 208
XI. The Minor Planets 229
XII. Jupiter 245
XIII. Saturn 268
XIV. Uranus 298
XV. Neptune 315
XVI. Comets 336
XVII. Shooting Stars 372
XVIII. The Starry Heavens 409
XIX. The Distant Suns 425
XX. Double Stars 434
XXI. The Distances ofthe Stars 441
XXII. Star Clusters and Nebulæ 461
XXIII.
The Physical Nature ofthe
Stars
477
XXIV.
The Precession and Nutation
of the Earth's Axis
492
XXV. The Aberration of Light 503
XXVI.
The
Astronomical
Significance of Heat
513
XXVII.
The Tides 531
Appendix 558
LIST OF PLATES.
PLATE
I. The Planet Saturn Frontispiece
II. A Typical Sun-spot
To face
page
9
A. The Sun " " 44
III.
Spots and Faculæ on the
Sun
" " 37
IV.
Solar Prominences or
Flames
" " 57
V. The Solar Corona " " 62
VI.
Chart ofthe Moon's
Surface
" " 81
B. Portion ofthe Moon " " 88
VII.
The Lunar
Crater
Triesnecker
" " 93
VIII. A Normal Lunar Crater " " 97
IX. The Lunar Crater Plato " " 102
X. The Lunar Crater Tycho " " 106
XI. The Planet Jupiter " " 254
XII. Coggia's Comet " " 340
C. Comet A., 1892, 1 Swift " " 358
XIII.
Spectra ofthe Sun and of
three Stars
" " 47
D.
The Milky Way, near
Messier II.
" " 462
XIV.
The Great Nebula in
Orion
" " 466
XV.
The Great Nebula in
Andromeda
" " 468
E. Nebulæ in the Pleiades " " 472
F. ω Centauri " " 474
XVI.
Nebulæ observed with
Lord Rosse's Telescope
" " 476
XVII. The Comet of 1882 " " 357
XVIII.
Schiaparelli's Map of
Mars
" " 221
LIST OF ILLUSTRATIONS.
FIG. PAGE
1. Principle ofthe Refracting Telescope 11
2.
Dome ofthe South Equatorial at Dunsink
Observatory, Co. Dublin
12
3. Section ofthe Dome of Dunsink Observatory 13
4. The Telescope at Yerkes Observatory, Chicago 15
5. Principle of Herschel's Reflecting Telescope 16
6.
South Front ofthe Yerkes Observatory,
Chicago
17
7. Lord Rosse's Telescope 18
8. Meridian Circle 20
9. The Great Bear 27
10. Comparative Sizes ofthe Earth and the Sun 30
11. The Sun, photographed September 22, 1870 33
12. Photograph ofthe Solar Surface 35
13. An ordinary Sun-spot 36
14. Scheiner's Observations on Sun-spots 38
15.
Zones on the Sun's Surface in which Spots
appear
39
16. Texture ofthe Sun and a small Spot 43
17. The Prism 45
18. Dispersion of Light by the Prism 46
19. Prominences seen in Total Eclipses 53
20. View ofthe Corona in a Total Eclipse 62
21.
View of Corona during Eclipse of January 22,
1898
63
22. The Zodiacal Light in 1874 69
23. Comparative Sizes ofthe Earth and the Moon 73
24. The Moon's Path around the Sun 76
25. The Phases ofthe Moon 76
26. The Earth's Shadow and Penumbra 78
27. Key to Chart ofthe Moon (Plate VI.) 81
28. Lunar Volcano in Activity: Nasmyth's Theory 97
29. Lunar Volcano: Subsequent Feeble Activity 97
30.
Lunar Volcano: Formation ofthe Level Floor
by Lava
98
31. Orbits ofthe Four Interior Planets 115
32. The Earth's Movement 116
33. Orbits ofthe Four Giant Planets 117
34. Apparent Size ofthe Sun from various Planets 118
35. Comparative Sizes ofthe Planets 119
36. Illustration ofthe Moon's Motion 130
37. Drawing an Ellipse 137
38. Varying Velocity of Elliptic Motion 140
39. Equal Areas in Equal Times 141
40. Transit ofthe Planet of Romance 153
41.
Variations in Phase and apparent Size of
Mercury
160
42. Mercury as a Crescent 161
43. Venus, May 29, 1889 170
44. Different Aspects of Venus in the Telescope 171
45. Venus on the Sun at the Transit of 1874 177
46.
Paths of Venus across the Sun in the Transits of
1874 and 1882
179
47.
A Transit of Venus, as seen from Two
Localities
183
48. Orbits ofthe Earth and of Mars 210
49. Apparent Movements of Mars in 1877 212
50. Relative Sizes of Mars and the Earth 216
51,
52.
Drawings of Mars 217
53.
Elevations and Depressions on the Terminator
of Mars
217
54. The Southern Polar Cap on Mars 217
55.
The Zone of Minor Planets between Mars and
Jupiter
234
56. Relative Dimensions of Jupiter and the Earth 246
57–
60.
The Occultation of Jupiter 255
61. Jupiter and his Four Satellites 258
62. Disappearances of Jupiter's Satellites 259
63. Mode of Measuring the Velocity of Light 264
64. Saturn 270
65. Relative Sizes of Saturn and the Earth 273
66.
Method of Measuring the Rotation of Saturn's
Rings
288
67.
Method of Measuring the Rotation of Saturn's
Rings
289
68. Transit of Titan and its Shadow 295
69. Parabolic Path of a Comet 339
70. Orbit of Encke's Comet 346
71. Tail of a Comet directed from the Sun 363
72. Bredichin's Theory of Comets' Tails 366
[...]... around the heavens, seems to have been first ascertained by astronomers whose names are unknown The skill ofthe early Oriental geometers was further evidenced by their determination ofthe position ofthe ecliptic with regard to the celestial equator, and by their success in the measurement ofthe angle between these two important circles on theheavensThe principal features ofthe motion ofthe moon... demonstrate the apparent annual movement ofthe sun There could be no rational explanation ofthe changes in the constellations with the seasons, except by supposing that the place ofthe sun was altering, so as to make a complete circuit oftheheavens in the course ofthe year This movement ofthe sun is otherwise confirmed by looking at the west after sunset, and watching the stars As the season...73 Tails ofthe Comet of 1858 367 74 The Comet of 1744 368 75 The Path ofthe Fireball of November 6, 1869 375 76 The Orbit of a Shoal of Meteors 378 77 Radiant Point of Shooting Stars 381 78 The History ofthe Leonids 385 79 Section ofthe Chaco Meteorite 398 80 The Great Bear and Pole Star 410 81 The Great Bear and Cassiopeia 411 82 The Great Square of Pegasus 413 83 Perseus and... Position ofthe Great Nebula in Orion 466 98 The Multiple Star θ Orionis 467 99 The Nebula N.G.C 1499 471 100 Star-Map, showing Precessional Movement 493 101 Illustration ofthe Motion of Precession 495 [Pg 1] THE Storyofthe Heavens "The Storyofthe Heavens" is the title of our book We have indeed a wondrous story to narrate; and could we tell it adequately it would prove of boundless interest and of. .. truths of nature, but, in the infancy of science, the men who made such discoveries as we have mentioned must have been sagacious philosophers Of all the phenomena of astronomy the first and the most obvious is that ofthe rising and the setting ofthe sun We may assume that in the dawn of human intelligence these daily occurrences would form one ofthe first problems to engage the attention of those... incurred the wrath of the Inquisition The structure ofthe human eye in so far as the exquisite adaptation ofthe pupil is concerned presents us with an apt illustration ofthe principle ofthe telescope To see an object, it is necessary that the light from it should enter the eye The portal through which the light is admitted is the pupil In daytime, when the light is brilliant, the iris decreases the. .. which the operation of condensing the rays of light is conducted by refraction The character ofthe refractor is shown in Fig 1 The rays from the star fall upon the object-glass at the end ofthe telescope, and on passing through they become refracted into a converging beam, so that all intersect at the focus Diverging from thence, the rays encounter the eye-piece, which has the effect of restoring them... movements ofthe planets It was found that they obeyed certain laws The cultivation ofthe science of geometry went hand in hand with the study of astronomy: and as we emerge from the dim prehistoric ages into the historical period, we find that the theory ofthe phenomena oftheheavens possessed already some degree of coherence Ptolemy, following Pythagoras, Plato, and Aristotle, acknowledged that the. .. Observatory for the equatorial telescope, the object-glass of which was presented to the Board of Trinity College, Dublin, by the late Sir James South The main part ofthe building is a cylindrical wall, on the top of which reposes a hemispherical roof In this roof is a shutter, which can be opened so as to allow the telescope in the interior to obtain a view oftheheavensThe dome is capable of revolving... comparison between the sighting of a rifle at the target and the sighting of a telescope at a star Instead ofthe ordinary large bull's-eye, suppose that the target only consisted of a watch-dial, which, of course, the rifleman could not see at the distance of any ordinary range But with the telescope ofthe meridian circle the watch-dial would be visible even at the distance of a mile The meridian circle . THE STORY OF THE HEAVENS PLATE I. THE PLANET SATURN, IN 1872. THE Story of the Heavens SIR ROBERT STAWELL BALL, LL.D. D.Sc. Author of "Star-Land" FELLOW OF THE ROYAL. from the Sun 363 72. Bredichin's Theory of Comets' Tails 366 73. Tails of the Comet of 1858 367 74. The Comet of 1744 368 75. The Path of the Fireball of November 6, 1869 375 76. The. explanation of the changes in the constellations with the seasons, except by supposing that the place of the sun was altering, so as to make a complete circuit of the heavens in the course of the