382 Mr. South's re-examination of the apparent distances 
No. XXXIV. R. A. 20 h 59 m ; Decl. 37 0 52' N. 
61 Cygni ; IV. 18 ;H. and S. 329. 
continued. 
Passy ; September 24 , 1825 ; Seven-feet Equatorial. 
6th and 7th magnitudes. 
Position = 2 0 50' nf I 7 Obs 
Distance — i^'. 6 Sg | 5 Obs. 
Position = 3 0 13' w/| 7 Obs. 
Distances: is".2o 8 j 5 Obs. 
South. 
Diff. — o° 46' 7 , 
Diff. = o ".697 j 1 
DifF. = 2 0 8' 7 n . _ 
jjjgr — j" r Captain Beaufort. 
Stars well defined aud very steady. 
Mean Result. 
Position 3 0 4' nf (63 Obs.) ; Distance 15".444 (45 Obs.); 
Epoch 1825.70. 
The result here given affords an extremely satisfactory 
verification of our former measures, and of the mean motion 
+ o°.730 assigned to this star. The interval of the epochs 
is 2.8 years, in which 2 0 f ought by computation to have 
been described, while by observation «f* 2 ° 1 5 / have been de- 
scribed. The distances too differ only by o".oi9, a quantity 
perfectly insensible. ( H. ) 
No. XXXV. R. A. 22 b 8 ™ ; Decl. 36° 51' N. 
1 Lacertse ? H. and S. 341. 
Double ; 8 th and 10th magnitudes ; small, blue. 
Passy ; September 29 , 1824 ; Seven-feet Equatorial. 
Position =■ 78° 33' sp I 5 Obs. I 
Distance = 1 s".434 | 5 Obs. J 
Diff. = i° 59 ' 
Diff. =o".48i 
difficult. 
Near this star, about 22 h 4' ± Right Ascension, and 36° 52' ± North Declina- 
tion, will be found a minute double star of the 1st or 2nd class ; but it is not 
measurable with this instrument, although the night is particularly favourable. 
Passy ; November 21 , 1824 ; Seven-feet Equatorial. 
7th and 10th magnitudes. 
s Obs! I Diff = o" 98 8 6 } Extreme b difficult. 
The small star is very obscure. 
Position =: 75° 4 sp 
Distance = i5 #/ .8o9 
