Full text: Elemente der physischen Astronomie (Dritter Theil)

355 
und diese sechs Tledingungsglciehungen reichen hin, die Werthe 
der sechs Gröfsen 
zu bestimmen. 
A° A* A 8 A 3 A 4 As 
S- 6. 
Wir wollen nun wieder zu der Gleichung (A) des Kap. II. 
zurückkehren. 
Es war 
u = ^1-f.e 2 -}-^- + eCo?( c r—w)—Cos3 (gv— 9 )^ -J-£u 
also ist auch 
1 . t y a ^ N 7 
»• J 
= 1 — 2 e 1 
2 
2 e Cos (cv—w) + ~ Cosa (gv— 9 ) 
Q r . 2 Se* 3<v s e 
-f- ' f- Cos 2 (cv—w) 4 - —Cos (er—w) 
2 2 
--- jcos‘[2(gv— 9 )—(cv—w)] -f- Cos [s(gv— 9 ) -f- (cv—w)]j 
! / C® «V® \ 
Ferner war h = b* ( 1 — —• ), also ist auch 
V 2 2 / 
! ( 1+ 5l + 2A 
cv® 3 e* j 
= 1—ue Cos (cv—w) + — Cos 2(gv— 9 ) — Cos 2(cv w) 
2 2 
+ Co<cv—w)— £<y’e jcos[2(gv—S)—(cv—w)] + 
Cos [2 (gv— 9 ) -j- (cv—w)] j 
und eben so wird man haben 
- 1 — ! — 3 ( e® 4 -—- + e Cos (cv—w)—^-Cos2(gv— 9 )^ 
a 3 u 3 V ‘ 4 4 / 
-j- 3 ^e* + ~~ + e Cos(cv— w)——-Cosa(gv— 9 )^ 
. Za
	        
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