Front matter
I
SI
If li i If I
Preface
" The science of Astronomy, conversant as it is with the sublimest natural phenomena, has ever engaged the attention of mankind, even when, from century to century, scarcely any new revelation of the skies rewarded the labors of the astronomer.
But at the present time, when discovery crowds upon discovery, and the whole field of astronomical research has been wonderfully enlarged, it has suddenly become invested with the charms and freshness of a new science ; and all classes of society listen with wonder and delight to the recital of the lofty truths and amazing facts which it unfolds.
In attempting, therefore, with many honored names, to cause Astronomy to descend from the dignified seclusion of the observatory, that she may walk as a familiar guest amid the lesser temples of knowledge, no apology is required for the motive that prompts the task how much soever it may be needed on account of the execution.
In the present treatise the author has not sought to adapt its subject to the youthful mind, by curtailing the science of its fair proportions, and omitting every thing that requires patient and earnest study ; but he has aimed to preserve its great principles and facts in their integrity, and so to arrange, explain, and illustrate them, that they may stand out boldly defined, and be clear and intelligible to the honest and faithful student, — this is all that can be done for a pupil, if a science is to be taught in its completeness and not in parts.
IV PREFACE.
The hill of science will always be a hill. Inipedi ments and obstructions may be removed and the ascent rendered easier, but the hill cannot be leveled, it must be surmounted.
Several peculiarities are contfined in this text-book, which it is thought will be of material service to the pupil in obtaining a knowledge o/ ihe science. The most important of these we shall now briefly notice.
I. It is usual, in most text-books on this science, to explain many astronomical phenomena by the apparent, and not by the real motions of the celestial bodies. In this treatise the opposite course is taken, wherever practicable ; the explanations being based upon the real motions of the heavenly bodies. By pursuing this method, the subsequent acquisitions of the scholar are built upon the truth itself, and not upon what appears to be true.
II. The mode of ascertaining the distances and magnitudes of the heavenly bodies is so simplified that any student, who understands the rule of proportion, can readily comprehend it.
III. Scientific terms and expressions are explained by foot notes on the pages in which they occur ; and in these notes are likewise embodied such illustrations and information as tend to elucidate the text.
In the preparation of this manual, the author has had recourse to numerous standard works upon Astronomy, and has brought up the subject to the present time. For information respecting recent astronomical discoveries, he is especially indebted to the treatises of Sir John Herschel and Mr. J. Russel Hind.
Hartford, Feb. 19th, 1855.
Contents
Preface.
Page. 3
INTRODUCTORY CHAPTER.
Chapter II. The Horizon
Sensible horizon, 33
Rotional horizon, 34
Plane of the horizon not fixed
in space, 35
Zenith and Nadir, 36
Changing aspect of the heavens arising from the rotation of
theearth, 36
Why the stars appear to describe circles, 38
Why these circles differ in size,
Changing aspect of the heavens arising from change in latitude
Circle of perpetual apparition,. .
Circle of perpetual occultation,.
Latitude of any place equal to the elevation of the pole of
39 41
V]
CONTENTS.
Chapter III
ON THE MODE OF DETERMINING THE PLACE OF A HEAVENLY BODY. Puge.
Pa*
Celestial sphere, poles,
and meridians, 46
Equators, 48
Virtieal Circles 49
The position of a star how determined, 49
Azimuth, amplitude, altitude,
and zenith distance, 50
Declination and right ascension, 51
Ecliptic, ". 53
Latitude and longitude, 53
The signs, 54
Zodiac 54
Chapter IV. Of Refraction
Refraction, 55
Variation of refraction in respect to altitude, 56
The effect of refraction on the position of heavenly bodies, . 58
Its effect on their declination and right ascension, 58
Refraction influenced by the temperature and pressure of the atmosphere, 60
Of parallax, 60
AND PARALLAX.
Parallax — how measured, 62
Variation in parallax — effect of
altitude, 63
Horizontal parallax, 63
Effect of distance, 63
Effect of parallax upon the true
position of a heavenly body, . 64 Its effect on right ascension
and declination, 64
Parallax — its value, 65
CHAPTER Y.
OF THE MEASUREMENT OF TIME.
Transit instrument, 66
Time occupied by the earth in performing one rotation —
how determined, 68
Standard unit of time, 70
Of the sidereal and solar day, 70
Inequality in the length of the
solar days, .75
Modes of reckoning time, 77
Apparent time, 78
Mean solar time, 78
Astronomical time, 78
Equation of time, 79
Chapter VI. Of The Annual Motion Of The Earth
Sun's apparent motion in declination, 81
Sun's apparent motion in right ascension, 82
Sun's apparent path, 83
Sun's apparent motion in declination explained, 83
Sun's apparent motion in right ascension explained, 86
Direction of motion in space explained, 86
Tropical year defined, , .
Its length — how found, The calendar,
Chapter VII, Of The Year
Sothic period,
The Mexican year,.
Greo-orian rule, . . .
90 90 93
CONTENTS.
Vll
Chapter VIII. Of The Precession Of The Equinoxes, Change Of The Pole-star
AND NUTATION.
Of the precession of the equinoxes,
Sidereal year,
Change of the pole-star,
Effect of precession on the right ascension and longitude of the stars,
Its effect on the declination and latitude,
Terrestrial latitude constant, . .
Page.
96 91
Relative positions of the signs and constellation of the zodiac
variable, 99
Cause of the precession, .. . 100
Influence of the sun, 100
Influence of the moon and
planets, 101
Obliquity of the ecliptic affected by nutation, 103
Chapter IX. Of The Earth S Orbit
Sun's apparent diameter, 105
Anomalistic year, 107
Apparent angular motion, 108
Variation in the earth's orbitual
velocity, 109
Form of the earth's orbit ascertained by angular velocities,. 110
Product of the square of the distance into the angular velocity — constant, 110
Kepler's laws, 112
Extent of the earth's orbit, 112
How ascertained, 112
Chapter X. Of The Seasons
The seasons, 115
Spring, 118
Summer, 118
Autumn, 120
Winter, 120
Polar winter — effects of refraction, 121
Twilight and its influence, .... 1 22
The cause of the unequal distribution of heat over the surface of the globe, 123 '
The summer of the southern hemisphere not hotter than that of the northern, 124
ELLIPTICITY OF THE EARTH'S ORBIT, ITS EFFECT ON THE SEASONS 125
Chapter I. The Sun
Real diameter of the sun, 12S
Its size, 130
Quantity of matter in the sun,. 131 Weight of bodies at the sun's
surface, 131
Solar spots, 133
Their size and number, 133
Motion of the spots, 134
Rotation of the sun, 136
Inclination of the sun's equator
to the plane of the ecliptic,. . 139 Physical nature of the sun, ... 140 Temperature at the sun's surface, 142
VI 11
CONTENTS.
CHAPTER II. Page
The distance of the moon, 143
Diameter in miles, 144
Moon's phases, 146
From new moon to the first
quarter, 146
From the first quarter to full
moon, 147
From full moon to the third
quarter, 147
From the third quarter to new
moon, 147
What the phases prove, 150
Sidereal month, 150
Lunar month, 150
Physical aspects of the
moon, 152
Lunar mountains, 153
The heights measured, 154
Names and heights of the lunar
mountains, 156
Lunar craters, 157
Lunar volcanoes 159
Page.
Lunar atmosphere, 160
The bulk, mass, and density of
the moon, 161
Moon's orbit, 161
Its figure determined, 162
Plane of the moon's orbit, 162
The line of the nodes, 163
The line of the apsides, 164
Increased apparent size of the
moon when in the zenith, . . 165 The moon always turns the
same face toward the earth, . 166
Libration in longitude, 167
Libration in latitude, 168
Diurnal libration, 169
Length of the lunar day, 169
The appearance of the earth as
seen from the moon, 170
Acceleration of the moon's motion in her orbit 171
The moon's path in space,. . . . 172
Chapter III. Eclipses Of The Sun And Moon
Lunar eclipses, 173
Of the earth's shadow, 175
Extent of shadow traversed hy
the moon, 177
Of the penumbra, 177
Duration of a lunar eclipse, ... 178
Red light of the disk, 179
Earliest observations of lunar
eclipses, 180
Eclipses of the sun, 180
Form of a solar eclipse, 180
Shadow of the moon, 181
Altitude of the moon, — its effect
on eclipses, 182
Total eclipses of the sun, 184
Duration of a solar eclipse,,. . . 186 Solar and lunar eclipses — points
of difference, 186
Frequency of eclipses,. ....... 187
Quantity of an eclipse,. ....... 187
The period of the eclipses — the
Saros, 189
CHAPTER IV central forces and gravitation.
Of gravity, 192
Its variation, 193
Universal gravitation discovered, 194
Universal gravitation defined,. . 197
Chapter V The Planets
Their distances, 198
Kepler's law of distances, 199
Bode's law of distances, 200
Of their magnitudes, 200
Division of the planets, 202
Inferior planets, 202
CONTENTS.
IX
Page.
Mercury, 203
His solar distance, 203
Orbit — inclination of its plane,. 204
Size — apparent — real, 204
Periodic time, 205
Rotation on its axis, 205
Phases, 206
Transit of Mercury, 206
Splendor of Mercury, 207
Mass and density, 208
Ancient observations of Mercury, 209
Venus, 209
Distance and periodic time, . . . 209
Apparent diameter, 209
Real diameter, 209
Rotation, 210
Orbit, — Inclination of its plane
to that of the ecliptic, 211
Phases, 211
Splendor of Venus, 212
Mass and density, 214
Atmosphere of Venus, 214
Transit of Venus, 214
The Earth, 217
Superior planets, 217
Mars, 218
Distance — Orbit — Inclination of
the plane of the orbit, 218
Real and apparent diameter, . . .218
Phases, 219
Physical aspect — Atmosphere,. 220 Rotation, — Inclination of the
axis,— Ellipticity, 221
Density and mass, 221
Intensity of solar light, 222
THE ASTEROIDS, 222
Ceres, 224
Pallas, 225
Vesta, 226
Astrea 227
Flora, 229
Metes, 230
Hygeia, 230
Parthenope, 231
Victoria or Clio, 232
Egeria, 232
Irene, 233
Eunomia, 233
Page.
Psyche, 234
Thetis, 234
Melpomene, , 234
Fortuna, 235
Massalia, 235
Lutetia, 235
Calliope 235
Thalia, .' 235
Themis, 236
Phoccea, 236
Proserpine, 236
Euterpe, 236
Bellona, 236
Amphitrite, 237
Urania, 237
Euphrosyne, 237
Pomona, 237
polymnia, » 237
The system pursued in naming
new planets, 238
Olber's theory, 238
Jupiter, 239
Periodic time — distance 239
Diameter — apparent — real . . . 239
Ellipticity— bulk, 239
Physical aspect of Jupiter —
Belts, 239
Rotation, 240
Velocity of rotation, 241
Mass— Density, 241
Satellites of Jupiter — their discovery, 241
Their magnitudes, diameters, distances, and periods of
revolution, 242
Kepler's laws — applicable to the
satellites — their rotation, .... 242 Transits and eclipses of the
satellites, 243
Velocity of light, 244
Saturn, 245
Distance — Periodical revolution
and inclination of orbit, 246
Form — diameter, 246
Bulk, diameter, intensity of
light, 246
Physical aspect — atmosphere,. . 246 Rotation and inclination of its
axis, 247
Ring of Saturn — its discovery, 247
Form — constitution,. 248
CONTENTS.
Page.
Rotation — Position — Inclination
to the ecliptic, 248
Phases of the ring, 249
Vanishing of the ring — Three
^auses, 250
Divisions of the ring, 251
Dimensions of the rings, 252
Satellites of Saturn, 253
Mimas, 253
Enceladus, 253
Tethys, 253
Dione, 254
Rhea, 254
Titan, 254
Hyperion, 254
Japetus, 255
Diameter of the satellites, .... 255 Ancient observations of Saturn, 255
Uranus or Herschel, 256
Aspect, — Diameter, — Mass, —
Density, 256
Page.
Rotation, 256
Distance, — Inclination of Orbit,
— Periodic time, 257
Satellites of Uranus, 257
Intensity of light, 258
Neptune,. 258
History of its discovery, 258
Name, — Diameter, — Mass, —
Density, 259
Orbit, — Inclination of orbit, — Distance, — Periodic time, . . 259
Intensity of light, 259
Has Neptune a ring, 259
The satellite of Neptune, 260
Real and apparent motions
of the planets, 260
Causes of the apparent motions, 261
Apparent motions explained,.. 261 The planets at times stationary, 262
Chapter VI. Comets
Their constitution, 262
Number of comets, 263
Splendor and size, 265
Velocity, 265
Temperature, 266
Comets shine by reflected light, 266 Orbits, — Perihelion distances, . 267 Inclination of the orbits, — Direction of motion, 268
Elements,— Identity, 268
Halley's comet, 269
Encke's comet, 270
Biela's comet, 270
Faye's comet, 271
De Vico's comet, 271
Comets of 1843, 272
Physical nature of comets, 273
Collision with the earth, 273
CHAPTER Vn.
Tides defined, 274
Cause of the tides, 276
Why high tides occur on opposite sides of the globe, .... 276 Why low tides occur on opposite sides*)f the globe, .... 277
Solar influence, 278
Spring and neap tides, 279
Time of the tide, 281
Priming or lagging of the tide, 282 Effect of declination on the
height of the tide,
Actual heights of the tide,
Derivative tides, .....' 284
No tides except on the ocean,
and on seas connected with
it,
282 283
CONTENTS.
Chapter VIII. Terrestrial Longitude
Pa<je.
Longitude ascertained by four
methods, 28G
By chronometers, 286
By eclipses,
By the electric telegraph, By the lunar method,
XI
Page.
287 288 288
Chapter I. Of The Fixed Stars In General And The Constellations
The fixed stars,
Magnitudes,
Number of stars, .
Distance of the fixed stars, ....
Parallax and distance of Alpha
Centauri,
Parallax and distance of 61
Cygni,
Nature and intrinsic splendor
The constellations, .
Their use,
290 290 291 292
295 295
The stars in the constellations,
— How designated, 296
Principal constellations, 296
Constellations north of the
zodiac, 296
Constellations of the zodiac, . . . 297 Constellations south of the
zodiac, 297
How to study the heavens, .... 298
The celestial globe, 298
Star maps, ^300
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