Full text: Elemente der physischen Astronomie (Dritter Theil)

(t—rh) 
■ | |E j ■ Ift 
e Cos [2 (v —mr) -j- (er—w')]. 
■ ' • iiili sr.ll 
ne* 
2 (2 —3 m) 
e* 
— Cos [2 Cr—mr)—(c'mr—w')] 
T(2—ml ^° S —■ rni ^ "f" (c'mr-w')] 
Y. Endlich ist noch aus dem in P. entwickelten Ausdrucke 
1 s 
h* Vdu/ h 3 u Vds/ 
das Glied — 
h 3 (i-J-s 3 )l 
1 . . . 1 
r [» — I7 2 Sin* (gn — S}] wofür wir hier hlofs setzen 
h h
	        
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