i6'o Mr. South’s observations of the apparent distances 
No. DCVIII. continued. 
Passy ; March 29, 1825 ; Seven-feet Equatorial. 
9th and 10th magnitudes. 
5 Obs! | Diff! = o°.745 } Excessively difficult. 
These observations, particularly of distance, do not accord so well as might 
be wished ; the star however is one which presents considerable difficulty : this 
circumstance must plead their excuse. By allowing all the measures equal weight, 
I apprehend we shall not err much from the truth, when we give as the 
Mean Result. 
Position 26° i' nf (24 Obs.) ; Distance 3".632 (21 Obs.); 
Epoch 1825.20. 
This star offers not the least evidence of change either in 
position or distance. The angle of 1782 differs only 31' from 
that here assigned; and the distance (2 diameters) for stars 
of this magnitude may (from centre to centre) amount to 
about 4". ( H.) 
Position == 24 0 28 nf 
Distance 1= 4".255 
No. DCIX. R. A. io h 22 m ; Decl. 22 0 58' N. 
Struve, 364 ; Hist. Gael. 150. 
Double; 9th and 9 x - magnitudes, and bear a very tolerable 
illumination. 
Passy ; February 9, 1825 ; Seven-feet Equatorial. 
Position rr 65° 50' sf j 5 Obs. Diff. =r o° 48' 7 
Distance — I4".588 j 5 Obs. Diff. = ‘ 
Passy; February 28, 1825 ; Seven-feet Equatorial. 
9th and 9| magnitudes. 
Position = 65° 51 ‘ sf 
Distance — 14". 090 
5 Obs. 
5 Obs. 
Diff. r= o° 24' 7 
Diff. = o".649 3 
Passy ; March 10, 1825 ; Seven-feet Equatorial. 
9th and 9| magnitudes. 
Position rr 64° 50' a f 
Distance zz 13". 938 
5 Obs. 
5 Obs. 
Diff. = o° 38' 7 
Diff. = o".649 5 
Mean Result. 
Position 65 0 30' sf{ 15 Obs.) ; Distance i4 /r .205 (15 Obs.) ; 
Epoch 1825.09. 
