Lockyer, Norman, Sir, 1836-1920 · London : Macmillan and Co. · leaf 219
p, theends of which are repre-sented by the stationarypoints. ]\Ioreover,itwillbe seenthat the planet during thetime was north of theecliptic, or in that part ofits orbit situated abovethe plane of the Earthsmotion round the Sun,and that the north lati-tude was increasing. Still,for all this, it… … Fig. 35.—Saturns apparent Path from1862 to 1865. (Proctor.) APPARENT MOVEMENTS. i«5 the equator. Let this be compared with what was saidabout the motion of the Moon in Art. 370, and it willbe evident that when on the meridian the planets height
Astronomy · Solar system
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