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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 271

An illustration from Astronomy for the use of schools and academies, 1882, leaf 271
piter varies from about fiftyseconds to about thirty seconds. His apparent size at hisextreme and mean distances from the earth is shown inFig. 273. Jupiter shines with a brilliant white light, which exceedsthat of every other planet except Venus. The planet is,of course, brightest when near… … Fig. 274. lution, or a complete revolution around the sun, his orbitalmotion being at the rate of about eight miles a second.His synodieal period, or the time of his passage from oppo-sition to opposition again, is three hundred and ninety-eightdays. 253. The Teleseopie Aspeet of Jupiter. — There…

Astronomy

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