Öebon.
Bestimmung des Azimuthes.
55
Object
Kreislage
Ulirzeit
Kreisablesung
wegen des Run
corrigiert
Correction
wegen
Neigung
Azimuth
des Sternes
Südpunkt
der
Kreistheilung
Azimuth
des Objectes
exclusive
Correction der
Collimation
1890. Mai 31. p
m.
« = l h 17 m 53*0; 3 = + 88° 43’ 3*7;
a? = —6 m 33 ? 6;
Tillenborg (Heliotrop)
L
112° 1’ 3 ,; 0
Polaris
W
10 h 49 m 33 ? 0
208 46 1-3
— 4’o
1° 13’ 22’-3
29° 59' 19*1
82° 1' 43*9
V)
0
10 53 9-0
28 47 6-3
— 1-8
1 11 54-5
209 58 59-0
57-5
Tillenberg (Heliotrop)
E
292 0 56-5
Mittel = 82° 1' 50*70
A a" = — 0-027 A a" 4-0-926 A <T
1890. Mai 31. p.
m.
« = l lL 17 m 53 ? 0; 3 = + 88° 43 ’ 37;
x = — 6 m 33'6;
Tillenberg (Heliotrop)
R
22° 1’ 48 J 2
Polaris
0
ll 11 3 m 1 ? 0
118 52 8 ? 6
— l f 2
1° V 48’’6
299° 59’ 55-9
82° 1’ 52*3
V)
w
11 7 17-0
298 54 9-3
4- 1-0
1 6 0-1
120 0 10-4
49-1
Tillenberg (Heliotrop)
L
202 1 59 5
Mittel = 82° 1’ 50*70
A«” = — 0-028 A a" 4-0*854 A 8"
1890. Juni 1. a.
m.
a = 1 U 17 m 54 ? 4; 3 = 4- 88° 43 ’ 3 3;
x — — 6 m 32'0;
Tillenberg (Heliotrop)
R
262° 2’ 43-8
Polaris
0
22 h 40 m 28 ? 0
1 20 53-0
4- 3 0
1° 20’ 9 v 6
180° 0' 46*4
82° 1’ 57*4
n
w
22 44 42-5
181 19 22-9
4- 7-5
1 18 28-0
0 1 2-5
48-7
Tillenberg (Heliotrop)
L
82 2 51-2
•
Mittel = 82°-l' 53*05
A a’ = 4- 0-027 A a" — 1-052 A o N "
1890. Juni 1. a.
m.
a = l h 17 m 54 ? 5; 3 = 4- 88° 43' 3*4-,
x= — 6 ,n 32 ? 0;
Tillenberg (Heliotrop)
I,
172° 2’ 17 v 0
Polaris
■ W
22 h 54 U1 27 ? 5
271 14 57-3
4- l r 9
1° 14' 27’’8
90° 0’ 31*4
82° 1' 45*6
??
0
23 0 48-3
91 11 50-9
+ 8-1
1 11 46-8
270 0 12-2
55-4
Tillenberg (Heliotrop)
R
352 2 7•6
Mittel = 82° 1’ 50*50
A a v = 4- 0-028 A a’ — 0'971 A <T
1890. Juni 1. a.
n.
a = l h 17 m 54 ? 5; 3 = 4-88° 43’ 3*4;
x = — 6 m 31 Ä 9;
Tillenberg (Heliotrop)
R
307° 4' 23 7
Polaris
O
23 h 18 m 26‘0
46 6 26•5
4- 3*8
1° 4’ 1*6
225° 2' 28*7
82° 1’ 55*0
n
W
23 23 26-5
226 4 17-6
4- 8-4
1 1 44-9
45 2 41-2
48-0
Tillenberg (Heliotrop)
L
127 4 29-2
Mittel = 82° 1' 51 * 50
A a" =4-0-030 A a" - 0-837 A
