Moulton, Forest Ray, 1872-1952 · New York, The Macmillan company · leaf 475
ecede farther andtheir paths becomemore curved. At acertain time the lat-eral disturbance of Sbecomes so great thatthe ejected materialrevolves around S in-stead of falhng backupon it. Let theorbits for this case be those marked! and 1 in Fig. 158, theformer being toward S, and the latter away from… … Fig. 158. — The origiu of a spiral nebiila. CH. XII, 249] EVOLUTION OF THE SOLAR SYSTEM 429 Now consider the location of all of the ejected materialat a given time after S has passed its nearest point to S.If it has been sent out from S continuously, it will He alongtwo continuous curves,…
Astronomy
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