432 Scientific llUdligencec 
Midnight at 
R. Asc. 
North 
Midnight at 
R. Asc. 
Nottli 
Gottingen, 
in Time. 
Decl. 
Gottingen. 
in Time. 
Decl. 
April 1. 
16i»44' 32" 
16° 21' 
June 4. 
161^12' 12" 
26° 11' 
9. 
16 48 16 
18 17 
12. 
16 6 0 
26 1 
17. 
16 46 20 
20 9 
20. 
16 0 44 
25 31 
25. 
16 42 56 
21 52 
28. 
15 56 40 
24 45 
May 3. 
16 38 8 
23 22 
July 2. 
15 55 4 
24 16 
11. 
16 32 20 
24 35 
10. 
15 52 56 
23 11 
19. 
16 25 44 
25 29 
18. 
15 52 8 
21 57 
16 18 52 
26 1 
30. 
15 53 28 
19 54 
*?. Geocentric Places of Juno, from May 5, to October 20. 1821. 
—The following geocentric places of J uno have been calculated 
by M. Nicolai of Manheim : 
Midnight at R. Asc. South 
Midnight at 
R. Asc. 
South 
Manheim. 
in Time. 
Decl. 
Manheim. 
in Time. 
Decl. 
May 5. 
20*' 20' 34" 
5° 46' 
Aug. 1. 
IQ*' 52 23" 
5° 17' 
13. 
20 24 14 
5 7 
9. 
19 45 52 
6 10 
21. 
20 26 43 
4 31 
17. 
19 40 15 
7 9 
29. 
20 27 53 
4 1 
25. 
19 35 56 
8 9 
June 2. 
20 27 57 
3 47 
Sept. 2. 
19 33 10 
9 9 
10. 
20 27 1 
3 27 
-10. 
19 32 6 
10 7 
•= 18. 
20 24 39 
3 14 
18. 
19 32 48 
11 0 
26. 
20 20 52 
3 12 
26. 
19 35 13 
11 4 
July 4. 
20 15 48 
3 20 
Get. 4. 
19 39 17 
12 3 
12. 
20 9 42 
3 40 
12. 
19 44 54 
13 8 
20. 
20 2 55 
4 11 
16. 
19 48 14 
13 19 
28. 
19 55 52 
4 53 
20. 
19 51 54 
13 32 
8. Astronomical Society of London, — The report of this flour- 
ishing institution, which has just been printed, is of th^ most 
gratifying nature, and will be read with the highest pleasure by 
every person who is attached to the study of astronomy, or who 
takes an interest in the public establishments of his country. 
The Council have ordered a die to be formed for striking 
medals in bronze, silver and gold, as a reward for any material 
discovery or improvement im^e science ; and they have speci- 
fied in their report the difihrent points in practical astronomy to 
which they wish the attenition of the candidates to be more par- 
ticularly directed. The Society’s Gold Medal and L. 21 will be 
given for the best paper on the Theory of the motions apd 
perturbations of the satellites of Saturn. The investigation to 
be so conducted, as to take expressly into consideration the in- 
fluence of the rings and the figure of the planet, as modified 
