9i Mr. South' s observations of the apparent distances 



No. CCCCXCVIII. R. A. p,^ 37" ; Decl. 22° 31' S. 



y Leporis ; V. 50. 



Double ; 5th and 8th magnitudes. 



Passy ; January 2, 1825 ; Seven-feet Equatorial. 



Position = y(f 42' «J9 I 5 Obs. DifF. = 0° 41' ) 



Distance= r 33".i82 I 6 0bs. I>\S. = i".\^^] 



Passy ; January 19, 1825 ; Seven- feet Equatorial. 

 6th and 8th magnitudes. 



Position = 79<* ^' np 15 Obs. 

 Distance = i' 34".5S3 \ 5 Obs. 



DifF. = 0° 24' ) 

 Diff.z: I ".370) 



Passy ; February 5, 1825 ; Seven-feet Equatorial. 



5th and 8th magnitudes. 

 Distance = i' 33".928 | 5 Obs. | DifF. = o".745 



Mean Result. 

 Position 79° 25' np (lo 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. CCCCXCIX. R. A. 5^ sS'" ; 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 = 68"> 25' sp or «/ 1 5 Obs. DifF. = 2° 49' | 



Distance = i".65 1 j 2 Obs. DifF. = o".474j 



Blackman-street ; March 12, 1824 ; Five-feet Equatorial. 



Equal ; each of the 8th magnitude. 



Position =70° 13' 50 or 7*/" c Obs. DifF. = «• 6' ) ,, 



Distance = i".655 5 Obs. DifF. =z o".569 \ ^^^ unsteady. 



These stars are separated with 133, but are best observed with 303 ; the night is 



very clear. 



