192 Mr. Herschel's and Mr. South’s observations of the apparent 
Position. 
31.10 
3 i- 7 
29.20 
29.36 
29.16 
30.18 
29.31 
30-35 
3°- I 5 
30.57 
31.12 
31.Z0J 
y s 
Mean — 30.23 
Position. 
H 
31.20 
3 1 -35 
31 - 35 
3 2 - 10 I 
32. oj 
31. JO'S 
32. o I 
32.20 )>S 
31.22 
32. O^ 
Mean — 31.45 
Stars beautifully 
Distance. 
Parts. 
56. S') 
54 - 8 
53 - o 
5 2 - 5 
57 - ° U 
56. 7 r 
5 6 - 3 
55 - 7 
55. 2 
54 - 5 j 
Mean 55.25 
Z r — 0.84 
54.41 
k Bootis continued. 
June 21, 1822. 
Five-feet Equatorial. 
sp 
Position = 30° 23' 
Distance = i2 // .646. 
April 7, 1823. 
Five-feet Equatorial. 
5 and 7 magnitudes. 
S P 
Position = 31° 45' 
Distance = 13". 129. 
steady, and well defined. 
Distance. 
Parts. 
40. 3 l 
42. 1 
40. 4 
42. 8 
41. 7 
40. o y s 
43 - 8 
41. 5 
4 i. 3 
41. 1 
4 >- 7 J 
Mean r= 41.52 
Z — — 1.48 
40.04 
Distance. 
Parts. 
43. o') 
39 - 1 I 
41. 8 J>H 
39- o 
41. oj 
43 - o') 
42. o 
40. 7 
Mean = 41.33 
Z — + 0.24 
4* -57 
July 6 . 1823. 
Seven-feet Equatorial. 
by daylight. 
Distance — 13 // .o82, 
Stars very steady, measures highly satis- 
factory. S. 
NB. This set of measures was taken to 
settle the discordance in the observations 
of distance. 
