380 Mr. Herschei/s and Mr, South’s observations of the apparent 
Position. 
o a e 
90—14.35-] 
14.20 
14- 3 r-S 
*4- S 
>3-5°J 
Mean — 14. 1 1 
33 Pegasi continued. 
September 17, 1823. 
Five-feet Equatorial. 
6 and 9 magnitudes. 
np 
Position = 75 0 49' np 
Distance = 56". 020. 
Mean. 
Distance. 
Parts. 
*7 8- 3 
179- 3 
1 79- 4 
178. 2 
178. o 
5>s 
Mean zz 178.64 
Z — — 1.26 
I77-38 
Position 7 5 0 45' np ; Distance 56". 045 ; Epoch 1823.71. 
1783.62 ; Position 89° 12 ' nf-. Distance 45 ''.05 ; H. Cat. 1785. 
The proper motions assigned by Piazzi to this star are 
+ 0" .40 in R. A., equivalent to 0".%% on the parallel, and 
— o",oi in declination. In 40 years therefore it should have 
moved 15". 2 from its place in a direction almost exactly co- 
incident with the parallel, and supposing the small star at 
rest, and the position of 1783 correct, the angle at present 
should be 75 0 38', coinciding exactly with the observed. The 
proper motion of this star appears therefore to be well es- 
tablished in fact and correct in quantity. 
No. CCCXLIII. R. A. 22 h i6 m ; Decl. 65° 50' N. 
Position. 
1789. 216 ; Struve, 751 ; 
9 and 9^ magnitudes. 
Distance. 
O of 
October 16, 1823. 
Parts. 
NO 
0 
1 
00 CO 
On On 
O O 
1 
Five-feet Equatorial. 
II. 2~ | 
13. O 
85 45 
> s sf 
II. 5 
86.42 
IO. 7 
85 - 54 J 
Position = 3 0 54' sf 
"• 3 . 
Mean — 86. 6 
Mean ~ 11.54 
Distance = 3". 7 11. 
Z ZZ + 0.31 
n.75 
