92 
Mr. South’s observations of the apparent distances 
No. CCCCXCVIII. R. A. 5 h 37 * ; Decl. 22° 31' S. 
y Leporis ; V. 50. 
Double ; 5th and 8th magnitudes. 
Passy ; January 2, 1825 ; Seven-feet Equatorial. 
Position = 79 0 42' tip I 5 Obs. Diff. zz o° 41' ) 
Distance = 1' 33 ".i 82 | 6 Obs. Diff. zz 1". 154) 
Passy ; January 19, 1825 ; Sevenfeet Equatorial. 
6th and 8th magnitudes. 
Position = 79 0 9 'tip I 5 Obs. Diff. zz o° 24' ) 
Distance = \' 34". 553 | 5 Obs. Diff. zz i".37o) 
Passy ; February 5, 1825 ; Seven-feet Equatorial. 
5th and 8th magnitudes. 
Distance zz 1' 33". 928 | 5 Obs. J Diff. zz ©".745 
Mean Result. 
Position 79 0 25' np (10 Obs.); Epoch 1825.03 ; 
Distance 1' 33".844 (16 Obs.); Epoch 1825.05. 
Sir W. Herschel has no measures of this star, and there 
is even a doubt of its identity with V. 50. (H.) 
No. CCCGXCIX. R. A. 5 h 38” ; Decl. 6° 23' N. 
52 Orionis ; Struve, 207 ; I. 20. 
Double ; equal ; each of the 8th magnitude. 
Blackman-street ; March 6, 1824 ; Five-feet Equatorial. 
Position zz 68° 25' sp or nf \ 5 Obs. | Diff. = z° 49' ) 
Distance zz i". 65 1 j 2 Obs. [ Diff. zz ©".474 ) 
Blackman-street ; March 12, 1824 ; Five-feet Equatorial. 
Equal ; each of the 8th magnitude. 
Position — 70° 13' sp or nf 5 Obs. 
Distance zz 5 Obs. 
Diff. zz 3 0 6' } v , 
Diff. zz o". 5 6 9 ^ ^ er 7 unsteady. 
These stars are separated with 133, but are best observed with 303 ; the night is 
very clear. 
