Full text: Bahnbestimmung der Planeten und Kometen

Methoden der ersten Bahnbestimmung. 
A 
2.266770 
2.407700 
2.596190 
v 2 
10.34328 
10.59382 
10.82702 
x' 
- 3- io 95 2 7 
-3-I7I734 
— 3.222828 
y' 
+ 0.374756 
+ 0.231208 
+ 0.0962614 
z' 
+ 0.730531 
+ 0.693165 
+ 0.656608 
Y 
3.216097 
3-254815 
3.290444 
c) Das Verbesserungsverfahren. 
A A 
0+1308 
0+1389 
0+11498 
t° 
20.35757 
37-385I3 
53-32923 
t° —1° 
15.94410 
32.97166 
17.02756 
T° 
0.274272 
0.567182 
0.292910 
Yl% 
0.483570 
0.516430 
X 2 
21.4091 
21.1196 
20.9234 
X 
4.62700 
4-59561 
4.57421 
^T 02 
0.09x9418 
0.393183 
0.104862 
2 (3-x + r + r) 
233523 
228.922 
225.628 
9* 
0.0003937 
0.0017175 
0.0004648 
y 
1.0003577 
1.0015587 
1.0004224 
y2 : yi 
1.0012006 
n-y 3 
1.0011358 
Yl-I 
0.484151 
n 3 
0.517017 
Diff. 
— 1 
Diff. 
+ 2 
(vili) 
(IVa) 
(IX) 
(X) 
Würde man die bisherigen Resultate zur Nachrechnung der mittleren 
Beobachtung nach Gl. (XII) benutzen, so erhielte man für die Ab 
weichungen da und dö im Sinne Beobachtung minus Rechnung die 
Beträge: da.— — o"i, dd= -\-o"i. 
Vi 
0.020019 
v 3 
0.020225 
+ 0.005072 k° = — 0.291623 n\ -f- 0.3x6620 — 0.315693 n\ 
+ 0.005072 1° =+0.291623^1 + 0.315693 v 3 
Ai = 2.4777 — 2.4099 ~ 
r% = i.002516 + 1.575897 Ai + Al 
Ai 
2.4078 
1 
3448405 
r 2 
3-254913 
i : r\ 
0.0289989 
Vi'.rl 
0.000581 
v 3 \v\ 
0.000587 
Yli 
0.484x51 
Yl 3 
0.517017 
niAi 
1.097481 
yi 3 A 3 
1.342348 
A 
2.266816 
2.407800 
2.596332 
Y 2 
10-34357 
10.59446 
10.82793 
Y 
3.216142 
3-2549I3 
3.290582 
X' 
- 3109570 
— 3.171826 
— 3.222958 
y' 
+ 0.374764 
+ 0.231228 
+ 0.0962937 
z' 
+ 0.730545 
+ 0.693198 
+ 0.656655 
YiY 3 
10.58298 
x'i*3 + yiy3 + z t z 3 
10.53782 
(XI) 
(Va) 
(Via) 
(Vila) 
(Villa)
	        
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