A. Wedemeyer: Definitive Bestimmung der Bahn des Kometen 18991 (Swift).
27
1899
Mittlere Zeit
Berlin *
Komet — Stern
; a app. &
in a j in d
5 app. &
Bar.
in а in 6 in
B. —R.
a in S
Rom (Collegio Romano).
A. N. 3554. Beobachter: E. Millosevich. Instrument: 10 zöll. Refraktor (Fadenmikrometer).
März 6
7 b 6"’33?4
66
-3'" 3?I7
—0' 2878
3 ll 3S ra 5 I -25
-24°43' o78
+0)34
+9.4
+o?29
-7-0
i5
7 15 51-4
35
+2 18.32
-6 59-5
2 59 46.93
— 13 8 29.0
+0.39
+6.9
+0.06
+4.3
i7
7 io 52.3
33
-i 45 01
+5 23.4
2 52 54.31
-10 59 45.9
+0.39
+6.5
-0.32
+4-8
Strassburg.
A. N. 3572, 3617. Beobachter: H. Kobold. Instrument: 18 zöll. Refraktor.
März 6
7
47
’ig?2
63
+0
'36165
+
3' 37-9
«»1
Ù
3S'
"41-07
-24° 40' i9’.'6
+° s 35
+9-7
-0*69
+ 5-6
6
7
47
I9.2
64
+0
1 5S3
+
6 19.i
3
38
41.47
-24
40
19.9
+0.35
+9-7
-0.29
+ 5-3
I I
7
29
30.2
51
-O
13-69
+
3 ''.9
3
>5
514
-'7
52
279
+0.34
+8-5
-0.00
+ 7-6
I I
7
29
30.2
52
— I
1.67
+
О 44.О
3
15
5.05
-17
52
28.2
+0.34
+8-5
-0.09
+ 7-3
12
7 3 6 512
4S
— I
34.05
+
3 44-7
3
IO
5916
— l6
37
27.9
+0-35
+8.0
-0.33
+ '7
'3
7
41
55-2
45
+o
0.S7
—
6 35.0
3
7
4.46
-'5
25
3.8
+0.36
+7.9
-0.14
+ 3-7
и
7
44
35-2
41
+0
46.01
—
6 154
3
3
I9.2O
-14
'4
55-3
+О.36
+7-7
—0.14
+ 0.8
1 5
7
52
38.2
35
+2
'2.57
—
5 '9-7
2
59
41.18
— *3
6
49.2
+0.37
+7-4
—0.27
+ 2.4
15
7
52
38.2
39
-O
49-'4
+
0 10.5
2
59
41.29
-'3
6
53-4
+0-37
+7-4
—0.16
- I.S
16
7 42
34.2
34
+0
44 59
—
2
56
'3-67
—
+0.36
—
+ 0.22
—
17
7
47
33-2
33
— I
49АЗ
-I-
7 1.6
2
52
49-49
-10
58
7-7
+0.36
+7-1
- O.06
- 1.9
Mai 13
12
33
12.2
304
-5
3-29
+
5 '7-7
25
14
47.06
+35
53
44.2
—0.60
+9-2
+О.77
— 2.6
>3
12
33
12.2
300
— I
44.20
—
3 7-0
23
14
46.89
+35
53
42.9
—0.60
+92
+O.60
- 31
17
12
40
9.2
2S6
—О
54.56
—
5 5'-S
22
44
I 3-3 I
+4'
59
52.З
—0.7S
+S.6
+О.9З
- 36
17
12
40
9.2
285
+0
56.S3
+
О O.5
22
44
'3-43
+4'
59
52.7
-0.78
+8.6
+ I.05
— 3.2
27
IO
16
26.2
247
— 3
7.67
-
2 54-5
20
6
52.27
+56 26
50.5
- I.2S
+6.3
+ I.32
+ 5-5
27
IO
16
26.2
246
+1
33-5 1
+
3 48.6
20
6
52.43
+56 26
^2.2
-1.2S
+6.3
+ I.48
+ 7.2
3 1
9
55
53-2
236
~3
38.19
—
' 33-4
iS
27
I4-S3
+56
56
25.4
-1.17
+2.7
+ О.78
+ 13.6
3'
9
55
532
234
—2
6.99
+
I 7.9
iS
27
14.96
+56
56 24.S
-'■17
+2.7
+О.91
+'3°
Juni I
IO
14
I4.2
231
-5
2I.92
+
1 33-4
iS
2
55-69
+56
l6
3.6
-0.99
+ 1.2
+О.48
+ '4-5
5
IO
40
46.2
212
-5
iS.10
4-
2 52.9
16
43
10.44
+5'
20
45.4
-O.4O
—0.2
-О.46
+ '4.4
7
IO
13
0.2
201
-4
iS.72
I 17.2
16
'4
24.0S
+4S
12
21.0
-0.32
+0.5
-О.57
+ 131
7
IO
13
0.2
198
+ 1
49.61
+
0 30.2
16
'4
2413
-I-4S
12
21.3
-0.32
+0.5
-О.52
+'3-4
8
IO
33
512
I92
-2
ii.28
+
3 1S.1
16
2
O.4O
+46 32 40.6
- 0.16
+0.6
-О.32
+ 5-0
8
IO
33
51.2
1S9
+0
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4 4-S
16
2
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+46 32 46.2
—0.16
+0.6
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+ 10.6
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IO
5
1.2
1S2
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45.46
+
3 '3-2
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4'
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+43
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36.2
—O.I4
+1-3
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+".3
12
9
55
1.2
177
— I
15.76
—
2 37 '
'5
25
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+40
12
34.7
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+ 1.8
— О.81
+ 9.6
16
11
6
28.2
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—
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59-27
+34 29
50.1
+0.21
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+ 8.6
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II
15
33-2
169
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7.92
+
8 6.6
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О
57.22
+34
29 15.S
+0.23
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—О.96
+ 3-7
17
IO
44
30.2
165
— I
48.90
—
3 55-8
'4 56
28.26
+33
'4
4S.2
+0.17
+2.9
-О.74
+ 6.6
19
IO
43
13.2
l6l
+1
55.88
+
i 40.5
14 4S
3*7 l
+3°
52
22.2
+0.18
+3-2
—О.87
+ 6.0
27
IO
47
41.2 ,
'52
—О
35-31
—
6 31.s
'4
2S
2.S3
+23
l6
I 3 I
+0.22
+3.8
—О.62
+ 30
Juli 8
11
16 4S.2
71
+7
45-67
4-
6 23.4
'4
'5
41.66
+16
'4
30.7
+0.23
+3.8
-О.47
+ '-3
8
II
43
51.2
72
+7
27.92
—
7 5-'
'4
'5
40.97
4-16
'3
58.2
+0.25
+3-9
— О.42
+ 3-9
IO
IO
21
52.2
114
— I
22.О7
—
5 '1-3
'4
'4
33-S2
+15
'5
54.4
+0.19
+3-5
-О.58
+ 1.6
IO
IO
21
52.2
99,
-и
24.39
—
5 42.8
'4
'4
33-9°
+15
'5
53-6
+0.19
+3-5
-O.5O
+ 0.8
12
IO
20
1.2
9 S
+0
37-34
—
2 12.6
'4
'3
38.77
+ '4
'9
56.S
+0.19
+3-4
—О.48
- '-5
3 1
IO
6
27.2 1
95
— О
8.52
4-
2 I4.O
'4
12
40.26
+ 7
41 46.6
+0.16
+2.9
-0-35
+ 6.2
Aug. i
IO
7
0.2
120
-4
3MS
—
2 '9-5
'4
12
5319
+ 7
25
30.5
+0.16
-f-2.8
— O.4O
+ 0.7
IO
IO
6
I9.2
S7
+3
26.60
i 53-2
'4
*5
36.20
+ 5
'3
4-5
+0.15
+2.6
—0.S4
+ 2.5
Mai 13. A. N. 3617 logp\a lies 9 )г 641 statt 9«941.
Juni 5. A. N. 4617 logpbS „ 9«065 „ 9.065.
März 12. Komet in dichten Dunstwolken zuletzt ganz verschwindend.
März 17. Komet wegen Dunst und Nebel ziemlich schwach, zuletzt nur mit Mühe zu erkennen.
Juli 10. Kern nicht zu erkennen.
Juli 31. Beobachtung schwierig. Starker NO-Wind erschüttert das Rohr und macht die Vergleichung unsicher.
August 10. Beobachtung bei ziemlich dunstigem Himmel und häufigen Störungen durch das Licht elektrischer Scheinwerfer
sehr schwierig.