Elements of Astronomy ...: With Explanatory Notes, and Questions for Examination |
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Page vii
... and number , ...... 133 Inclination of the sun's equator to the plane of the ecliptic , .. 139 Physical nature of the sun , 140 Temperature at the sun's sur- face , .... ... 142 Page . The distance of the moon , .. 143.
... and number , ...... 133 Inclination of the sun's equator to the plane of the ecliptic , .. 139 Physical nature of the sun , 140 Temperature at the sun's sur- face , .... ... 142 Page . The distance of the moon , .. 143.
Page viii
... inclination of its plane ,. Page . The distance of the moon , .. 143 Lunar atmosphere , 160 Diameter in miles , 144 The bulk , mass , and density of MOON'S PHASES ,. 146 the moon , .. 161 From new moon to the first MOON'S ORBIT ,. 161 ...
... inclination of its plane ,. Page . The distance of the moon , .. 143 Lunar atmosphere , 160 Diameter in miles , 144 The bulk , mass , and density of MOON'S PHASES ,. 146 the moon , .. 161 From new moon to the first MOON'S ORBIT ,. 161 ...
Page ix
... inclination of its plane ,. 204 MELPOMENE , Real and apparent diameter , ... 218 Phases , Physical aspect - Atmosphere ,. 220 248 Distance , -Inclination of Orbit , 253 Name ,. MERCURY ,. 203 PSYCHE ,. ix Page . 234 His solar distance ...
... inclination of its plane ,. 204 MELPOMENE , Real and apparent diameter , ... 218 Phases , Physical aspect - Atmosphere ,. 220 248 Distance , -Inclination of Orbit , 253 Name ,. MERCURY ,. 203 PSYCHE ,. ix Page . 234 His solar distance ...
Page x
With Explanatory Notes, and Questions for Examination John Brocklesby. 248 Distance , -Inclination of Orbit , 253 Name , -Diameter , - Mass , 253 Orbit , -Inclination of orbit , - 254 Intensity of light , 254 Has Neptune a ring , .. 254 ...
With Explanatory Notes, and Questions for Examination John Brocklesby. 248 Distance , -Inclination of Orbit , 253 Name , -Diameter , - Mass , 253 Orbit , -Inclination of orbit , - 254 Intensity of light , 254 Has Neptune a ring , .. 254 ...
Page 17
... inclination between two lines that meet each other ; thus , in Fig . 2 the FIG . 2 . A D B E AN ANGLE . 1. The stars are frequently called orbs , from their round figures . Orbis , ( Latin , ) a circle . In what order are the subjects ...
... inclination between two lines that meet each other ; thus , in Fig . 2 the FIG . 2 . A D B E AN ANGLE . 1. The stars are frequently called orbs , from their round figures . Orbis , ( Latin , ) a circle . In what order are the subjects ...
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Common terms and phrases
altitude angular aphelion apogee apparent diameter apparent motion appear apsides ascertained asteroid astronomers atmosphere axis celestial equator celestial sphere centre changes circle circumference comet constellation craters degrees Describe difference direction discovered disk earth earth's orbit equal Explain from figure extent fixed stars globe Grammar heavenly body heavens hemisphere horizon hundred illumined inclination inferior conjunction J. R. Hind Jupiter latitude latter length libration longitude lunar eclipse magnitude Mars mean solar measured Mercury meridian miles moon moon's orbit mountains move nearly nebula nodes observations occur parallax passing penumbra perigee perihelion period planet position precession Prof quarter radius rays refraction respecting revolution revolve right angle right ascension ring rotation satellites Saturn seen shadow sidereal sidereal day solar day solar distance solar eclipse space spectator spots sun's surface synodical month tance telescope tides tion triangle velocity Venus vernal equinox visible west to east zenith
Popular passages
Page 296 - The fourth term is found by multiplying the second and third terms together and dividing by the first § 14O.
Page 24 - A sphere is a solid bounded by a curved surface, every point of which is equally distant from a point within called the center.
Page 164 - These phenomena do not, however, occur at every new and full moon ; and the reason is, that the plane of the moon's orbit is inclined to that of the ecliptic, and that these two planes' meet one another only in their line of common section, which passes through the centre of the earth.
Page 305 - On a careful re-examination of the heavens, too, and a comparison of catalogues, many stars are now found to be missing-; and although there is no doubt that these losses have often arisen from mistaken entries, yet in many instances it is equally certain that there is no mistake in the observation or entry, and that the star has really been observed, and as really has disappeared from the heavens...
Page 24 - A SPHERE is a solid bounded by a curved surface, every part of which is equally distant from a point within, called the centre.
Page 162 - In some of the principal ones, decisive marks of volcanic stratification, arising from successive deposits of ejected matter, and evident indications of Lava currents streaming outwards in all directions, may be clearly traced with powerful telescopes.
Page 13 - Dodd, I find it greatly superior to all others which have come under my notice, in system, completeness, and nomenclature. The arrangement is natural, the system complete, and the nomenclature greatly improved. These improvements are not slight; they are fundamental— eminently worthy the attention of the mathematical teacher, and give a character of unity to the work which at once distinguishes it from all others on this subject.
Page 50 - ... the sun. More Accurate Computations. — A more accurate determination of the phases as visible at any point of the earth's surface may be obtained from the Besselian elements which are given for every ten minutes of Greenwich mean time. Their geometric signification is as follows: — Let us imagine a plane passing through the centre of the earth, perpendicular to the right line joining the centres of the sun and moon. This latter line is the axis of the moon's shadow, and the plane is called...
Page 51 - Circles are great circles passing through the zenith of an observer, and perpendicular to his horizon. The vertical circle passing through the east and west points of the horizon is called the Prime Vertical ¡ that passing through the north and south points coincides with the celestial meridian.
Page 318 - This is an irresolvable nebula, figured by Sir John Herschel, during his residence at the Cape of Good Hope. Its favourable position, as seen in southern latitudes, enabled Herschel to trace the outline of the nebula much farther than any preceding observer had done. The singular figure of this object seems to suggest some power of attraction operating on the particles of matter, or the...