2 go Mr. South’s observations of the apparent distances 
No. DCCXCIX. continued. 
Passy ; November 9, 1824 ; Seven-feet Equatorial. 
5 th and 7 th magnitudes. 
Diff. = o° 5' 
Diff. = o". 6 i$ 
| Hazy. 
Position = 30° 42' nf I 5 Obs. 
Distance = 2' 33". 325 | 5 Obs. 
Observed when i h 20' west of the meridian; night unfavourable; no measures of 
A C can be obtained. 
Measures of A C. 
Blackman-street; July 10, 1824; Five-feet Equatorial. 
5 th and 12 th, or 15 th magnitudes. 
Position = 50° 8' np [ 2 Obs. | Diff. — o° 45'. Excessively difficult. 
Th? extreme faintness of the small star renders observations of distance impracti- 
cable ; but I consider it less than that of A B. 
Mean Result. 
of A B. Position 30° 39' nf; Distance 2' 33". 170 ; 
Epoch 1824.68. 
of A C. Position 50° 8' np; Distance about minutes ; 
Epoch 1824.53. 
Sir W. Herschel has no measures of this star. (H.) 
No. DCCC. R. A. 2 i h 49™ ; Decl. 6i° 45' N. 
Struve, 734; 1789. 213. 
Triple ; A 6 j, B 7th, and C of the 12th magnitudes. 
Measures of A B. 
Blackman-street; July 11, 1824; Five-feet Equatorial. 
5 Obs. 
5 Obs. 
Three hours and a half east of the meridian, at the time of observation ; of A C no 
measures can be obtained. 
There are two sets of triple stars in the field ; the stars here measured are 
the two brightest. 
Passy ; November 16, 1824 ; Seven-feet Equatorial. 
Triple ; but the 3 rd star will not bear the least illumination. 
Position = 55°4 1 sf 
Distance = T 2''.82 6 
Diff. r: o° eg' ) , 
Diff. = o".65 9 * Very steady. 
Note . 
Position = 55° 39 ' s f 
Distance= i' 2".847 
5 Obs. 
5 Obs. 
Diff. = o° 46' 
Diff 
. = o° 46 < 
’. = o".8i7j 
Mean Result. 
of AB. Position 55°2i ' sf; Distance i'2".836; Epoch 1824.70- 
