51 I
Reduction 'Laerration f. w.Aequ. -- 4h-
6'56"6 - l"9 7 12,4 1,7 7 2S,4 1,5 7 44,s 1,3 A 0,6 i,i
8 16,6 - 0,9 8 32,4 0,7 8 47,9 0,4 9 3,2 - 021 9 18,2 f 0,1
9 3 2 8 f 0,4 9 4720 0,6
10 019 0,9 10 14,4 1,2 10 27,6 1,5
10 40,4 f 1,7 10 52,9 2,O
Nr. 351.
Ger. Aufat.
-,- 242'37'33'9 243 25 45,; 244 20 15,€ 245 20 45,3
a
246 26 47,a
247 37 46,C 248 53 1,5 250 11 51,1 251 33 33,C 252 57 24,1
254 22 47,4 255 49 S,E 257 15 59,3 258 42 54,l 260 9 32,:
261 35 37,t 263 0 56'1
31 2
Log. der v. d.Erde.
9,926756 9,942940
-- 9,958717 9,974022 9,9 8880 1
0,003010 0,0166?1 0,029620 0,04?008 0,05379€!
0,0 6 5 0 1 2 0,075676 0,085824 0,095487 0,104699
0,113493 0,121900
12hmittl BerLZeit -
16 17 I 8 !9 20
21 22 23 24 25
26 27 28 29 30
31 32
Entfernung. Y. d.Sonnc.
9,544629 -- 9,536809
9,539457
9,552137
9,572929
9,5 9 92 5 6
9,628(i84
9,659341
9,689966
2 8,47 2 23,87
2 51,53
+ 3 3,10 3 12,92 3 20,94 3 27,20 3 31,80
+ 3 34,90 3 36,68 3 37,35 3 37307 3 36,02
2 38,37
+ 3 34,33 3 32,12
Stiindliche Bcwegyng.
0,329 0,313
0,258
+0,223 0,186 0,149 0,112 0,080
+0,050 0,025
$-0,003 -0,014
0,029
-0,041 0,050
0,289
P -I+= 20 33 40,7 21 19 24,7 22 3 1 1 , O 22 44 49,5
-23 24 11,l 24 1 8,7 24 35 37,3
25 37 1,4 25 7 34,9
-26 3 59,4 26 28 33,O 26 50 47,7 27 10 50,O 27 28 46,9
-27 44 4526 27 58 53,4
1 56,64 0,093 1 51,95 0,102 1 46,53 0,111 1 41,31 0,119
- 1 35,44 +0,125 1 ?9,32 0,130 1 23,05 0,131
I 10,49 0,1119 I 16,74 0,131
- 1 4 3 7 $0,125 0 58'46 0,121 0 52,81 0,115 0 47,44 0,109 0 42,35 0,103
- 0 37,5H +0,096 i 0 33,12 0,090
Zeduction '. w.Aequ.
5 T 795 775 726 7,7
- 7,7 7,s 7,s 7,9 799
- 8,O 8 4 8,i 891 8,2
- 8,2 8,2
duszug eiiies Schreibens V O ~ Sir John HerscheZ an den Werrii Gelieimenrath Beer iincl dcii Herru Dr. MiidZer
T h e last astronomical novelty of the Southern hemisphere i s one of very great interest. The Star y Argus (marked in Bode's Map a s 7 Robur Caroli) has always hitherto been regarded a s a Star of the second niagriitude or a t most as (2 .1) During the former years 1 h a l e had it (as is were) contiriually under my eye, by reason of the great nebula which surrounds i t , and of which I have been taking most careful drawings. I have always considered it as (2.1) and never had reason to suppose it variable. In Noveniher 1837 I saw it a s usual. .Iudge of my surprise to find on the 16. 17. De- cember that it had suddenly become a Star of the first magnitude and almost cquat to Rigel. It continued to in-
crease. Rigd is now not to he comparcd to it, it e x c e e d s A r c t u r u s and is very nearly equal to OL Centauri, being a t thc moment when I write, the fourth Star in the heavens in order of brightneb.
J . 3'. PV. Her*scheL
A n ni e r k u n g .
Dies Schrciben i d ohne Datum, miifs aher nach anderen darin angefiihrten Umsthden in der Mitte ties Januars (1. J. geschrieben seyn. Sir John Herschel denkt im Mai w i d e r in England anzukommen.
s.
I n h a l t . Beobachtiingen von Mondsternen nuf der Hamburger Sternwarte. Elemelite d e s Doppelsterns ?I Coronae. Epheineride des Ponsschen Cometen fur 1838. Auszug cines Schreibens von Sir John Herschel a11 den Herrn Gelieimenretl~ Beer und den Herrn Dr. Miidler.
Von Herrn Ch. RurnX-er.
p. 303.
p. 297. p.. 303.
(S. Astr. Nachr. Nr. 353.) p. 311.
M o n a 1838. Juni 7.
