382 Mr, South's re'examination of the apparent distances 



No. XXXIV. R. A. 20^^ 59™ ; Decl. sT 6^' N. 



61 Cygni ; IV. 1 8 ;H. and S. 329. 



continued. 



Passy ; September 24, 1825 ; Seven-feet Equatorial. 



6th and 7th magnitudes. 



Position =s i"* 50' nf I 7 Obs. DiflF. = o® 46' ") <, 

 Distance = i5".689 | 5 Obs. | Diflr. = o" .697 ]^^^'^^' 



Position =: 3° 1 3' n/ 1 7 Obs. f DifF. = 2" 8' 7 ^ , . „ 

 Distances is".208 | 5 Obs. | Diff.= i".o34 i ^^P*^^" Beaufort. 



Stars well defined aud very steady. 



Mean Result. -s = n. 



Position 3° 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 

 + 0^.730 assigned to this star. The interval of the epochs 

 is 3.8 years, in which + 2° s' ought by computation to have 

 been described, while by observation + 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^ 8"» ; Decl. 36° 51' N. 



^,^ 1 Lacertse ? H. and S. 341 • 



Double ; 8th and 10th magnitudes ; small, blue. 



Passy ; September 29, 1824 ; Seven-feet Equatorial. 



Position = 78; 33' sp I S Obs. I Diff. = 1° 59'} Very difficult. 

 Distance = 15 .434 | 5 Obs. | Diff. =0 .481 3 ^ 



Near this star, about 22* 4' ± Right Ascension, and 36° 52' ± North Declina- 

 tion, will be found a minute double star of the ist 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 lOth magnitudes. 



Position = 75° 4' sp 

 Distance = i5".8o9 



^gb^: I SI i^-Jse I Ex.ren.el, difficult. 



The small star is very obscure. 



