Full text: Bahnbestimmung der Planeten und Kometen

14. Die Methode von Olbers. 
199 
]ri 
0.022802 
)r 1 
0.047038 
I: ]/r x 
9.977!98 
x: ]r 3 
9.952962 
Ctg | («3 - Mi) 
0.517461 
cosec i («3 — Ml) 
0.536627 
sin \v-i\jq 
8-559339 
)>i _r ctg ~ («3 — Mi) 
0.494659 
sec \ Vi 
0.000317 
Add. 
8.069750 
cos { vi: ]q 
9-977 i 98 
}V 3 1 cosec i (m 3 — Ml) 
0.489589« 
8.582141 
1: I? 
9.9775I5 
7®* 
2?i88o 
V? 
0.022485 
Vi 
4.3760 
v 3 
3871700 
CO 
36.1093 
q 
0.044970 
aaJ 
7.99621 
aaJ 
7.93024 
0700991 
0700852 
n 
5.11000 
t0 3 
35.98922 
tgi»? 
5.746423 
*87®! 
8.617183 
1:3 
9.522879 
1:3 
9.522879 
jtgi»? 
5.269302 
• jtgi»! 
8.140062 
Add. 
0.000212 
Add. 
0.016993 
8.582141 
tg|®3 
9.539061 
Summe 
8-582353 
Summe 
9-556054 
I.9I4934 
}'2: k 
I-9I4934 
M, 
0.497287 
M 3 
1.470988 
3 
? 2 
0.067455 
q* 
0.067455 
Mi g'lT I 
0.564742 
3.6706 
M 3 qH | 
I.538443 
34-5496 
T 
1-4394 
T 
1.4396 
(XIII) 
(XIV) 
(XV) 
e) Kontrolle durch Nachrechnung der mittleren Beobachtung. 
AA 
0.0089 
7 2 sin «2 cos i 
9.227891« 
/0 
*2 
20.0204 
Add. 
9.9I5I54 
T 
1-4395 
— i?2 sin (L a — ft) 
9.978779 
- Tj 
18.5809 
72 COS M 2 
9.787731 
1.269067 
Add. 
0.182722 
3 
i \q2 
M 2 
9.932545 
1.201612 
— i?2 cos (L 2 — ft) 
9.506298 
t lz V 2 
1078226 
ZI2COS ß 2 Sin (7.2 — ft) 
9.893933 
cos I l 2 v 2 
9.992206 
COS (¿2— ft) 
9.884392 
COS x /j 
9.984412 
A 2 cosß 2 cos (A 2 —ft) 
9 970453 
v 2 
2176453 
tg (Aa—ft) 
9.923480 
CO 
36.1093 
A2 — ft 
39 9 9783 ( XVI ) 
9.981149 
u 2 
57-7546 
2J2 sin (/? 2 ) 
sin «2 
9.927253 
cos (ß 2 ) 
9.895666 (XVII) 
7 2 
0.060558 
Az cos (/? 2 ) 
0.086061 
cos u 2 
9.727173 
tg (ßz) 
9.895088 
sin i 
9.993338 
(Az) 
35870275 
r 2 sin u 2 
9.987811 
(ßz) 
+38.1459 
cos i 
9.240080 « 
Az 
0.190395 
u 
20974298’ 
(Az)-L 2 
14875977 
ft 
318.0492 
sin ((Az) — Lz) 
9.716875 
Dz —ft 
251.3806 
tg (1ßz) 
9.895088 
sin (¿2-ft) 
9-976653« 
tg (/2) 
0.178213 
Rz 
0.002126 
tg /2 
0.178144 
cos (L 2 — ft) 
9.504172 « 
tg Jz - tg (/2) 
— 0.000069
	        
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