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Astronomy for the use of schools and academies (1882)

Gillet, J. A. (Joseph Anthony), 1837-1908, Rolfe, W. J. (William James), 1827-1910 · New York : Potter, Ainsworth, & Co. · leaf 248

An illustration from Astronomy for the use of schools and academies, 1882, leaf 248
owing to the greateccentricity of its orbit, its distance from the sun varies from about forty-three million milesat aphelion toabout twenty-eightmillion at perihe-lion. 217. Distance ofMercury from theEarth. — It is evi-dent, from Fig.251, that an infe-rior planet, likeMercury, is thewhole… … Freia Fig. 249. 226 ASTRONOMY. from the earth at inferior conjunction also varies considera-bly. Mercury is nearest to the earth when its inferiorconjunction occurs at its own aphelion and at the earthsperihelion. 218. Apparent Size of Mercury. — Since Mercurys dis-tance from the earth is variable,…

Astronomy

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