An Elementary Astronomy for Academies and Schools: Illustrated by Numerous Original Diagrams and Adapted to Use Either with Or Without the Author's Large Maps

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Huntington and Savage, 1849 - Astronomy - 243 pages

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Contents

Distances of the Planets from the Sun
25
Degrees Minutes and Seconds explained
26
Angular Distances Magnitudes c
27
The Sun as seen from the different Planets
28
Philosophy of the Diffusion of Light
28
Light and Heat of the several Planets
30
Magnitude of the Planets
31
Relative Magnitude of the Sun and Planets
32
Comparative Density of the Planets 17 Attraction of the Planets
33
Periodic Revolutions of the Planets 21 22
35
41
36
Diurnal Revolutions of the Planets
37
True Figure of the Planets
38
The Ecliptic 24 The Poles of the Ecliptic 25 Obliquity of the Ecliptic
40
NodesAscending and Descending 26 The Zodiac 27 Signs of the Zodiac
42
Transits
43
Transits of Mercury
44
Transits of Venus
45
Celestial Latitude 34 Celestial Longitude 36 Constellations of the Zodiac 37 The Suns Apparent Motion in the Ecliptic 32 Inclination of the Orbits of ...
46
Philosophy of the Seasons
47
Longitude of the Ascending Nodes of the Planets
48
48
48
Inclination of the Axes of the Planets to the Plane of their re spective Orbits
50
Seasons of the different Planets
51
Seasons of Venus 53 Seasons of Mars 54 Seasons of Jupiter 55 Seasons of Saturn Lesson 38 Successive Appearance of the Constellations in the Noct...
52
Disagreement between the Months and Signs
53
The Equinoxes 41 Precession of the Equinoxes
54
The Solstices
56
53 54 54 56 57 XXXXXXX8858 888865
59
67
67
Conjunctions and Opposition of Planets
69
Sidereal and Synodic Revolutions
70
Elongations of a Planet 59 When Planets are said to be Stationary
72
Direct and Retrograde Motions
73
Retrograde Motions of the Exterior Planets
74
Venus as Morning and Evening Star
75
Nature and Causes of Tides
92
CHAPTER III
93
Supposed Satellite of Venus 72 72 73 74 75 76
94
Other inequalities of the Tides
95
Changes or Phases of the Moon 94
96
Motion of the Apsides of the Moons Orbit
96
The Moons Path around the Sun
97
Revolution of the Moons Nodes around the Ecliptic 74 Sidereal and Synodic Revolution of the Moon 75 Revolution of the Moon upon her Axis 97 ...
98
The Moons Librations
99
Telescopic Views of the Moon
100
Physical Constitution of the MoonMountains Volcanoes At mosphere c
102
Moons or Satellites of Jupiter
104
Satellites of Saturn
105
Satellites of Herschel 84 Supposed Satellite of Le Verriers Planet 104
107
CHAPTER IV
108
Character Extent and Duration of Solar Eclipses 87 Eclipses of the Moon
110
122
120
Magnitudes Velocities and Temperature of Comets
132
Periods Distances and Number of Comets 100 Direction Orbits and Nature of Comets CHAPTER VII
134
Nature of the Solar Spots 102 Spots on the Suntheir Number
139
Magnitude of the Solar Spots 105 Revolution of the Sun upon his Axis
142
Direction Motions and Phases of the Solar Spots
143
Physical Constitution of the Sun
144
108
146
Motion of the Sun in Space 138 139 140 142 142
147
110
150
Laws of Planetary Motion
152
Miniature Representation of the Solar System
155
Were the Asteroids originally one Planet?
156
114
158
PART II
161
Number of the Fixed Stars
163
Distances of the Stars
164
Magnitude of the Stars
165
List of the Constellations 121 Description of some of the Principal ConstellationsZodiacal Constellations
166
Northern Constellations 123 Southern Constellations
167

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Page 160 - Canst thou bind the sweet influences of Pleiades, or loose the bands of Orion? Canst thou bring forth Mazzaroth in his season? or canst thou guide Arcturus with his sons?
Page 210 - The PRIME VERTICAL is that azimuth circle which passes through the east and west points of the horizon, and is always at right angles...
Page 148 - The radius vector (line joining the centre of the sun with the centre of the planet) of each planet sweeps over equal areas in equal times. (3) The squares of the periodic times (the periods of complete revolution round the sun) of nnv planets are proportional to the cubes of their mean distances from the sun.
Page 183 - This remarkable law of variation certainly appears strongly to suggest the revolution round it of some opaque body, which, when interposed between us and Algol, cuts off a large...
Page 181 - In such instances, the larger star is usually of a ruddy or orange hue, while the smaller one appears blue or green, probably in virtue of that general law of optics, which provides that, when the retina is under the influence of excitement by any bright, colored light ; feebler lights, which seen alone would produce no sensation but of whiteness, shall for the time appear colored with the tint complementary to that of the brighter.
Page 149 - On it place a globe, two feet in diameter; this will represent the Sun; Mercury will be represented by a grain of mustard seed, on the circumference of a circle 164 feet in diameter for its orbit; Venus a pea, on a circle 284 feet in diameter; the Earth also a pea, on a circle of 430 feet; Mars a rather large pin's head, on a circle of 654 feet...
Page 181 - Thus a yellow colour predominating in the light of the brighter star, that of the less bright one in the same field of view will appear blue ; while, if the tint of the brighter star verge to crimson, that of the other will exhibit a tendency to green — or even appear as a vivid green, under favourable circumstances.
Page 182 - ... a red and a green, or a yellow and a blue one — must afford a planet circulating about either; and what charming contrasts and "grateful vicissitudes," — a red and a green day, for instance, alternating with a white one and with darkness, — might arise from the presence or absence of one or other, or both, above the horizon.
Page 181 - It is by no means, however, intended to say, that in all such cases one of the colours is a mere effect of contrast, and it may be easier suggested in words, than conceived in imagination, what variety of illumination two suns — a red and a green, or a yellow and a blue one — must afford a planet circulating about either ; and what charming contrasts and

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