of the Georgian planet. 323 
1793, March 8, n h 21'. The first satellite is about 65° 
nf ; the second is 90° nf ; a third is about 75 0 nf. 
J The first was 37^° nf ; the second was 89! 0 nf ; the third 
was a star. 
1793, M ar °h 9, io h 35'. The first satellite is 85° nf ; the 
second is about 82° np ; a third is about 65° sp. 
J The first was 8o° nf ; the second 77^ 0 np; there is no 
subsequent observation of the third. 
1793, March 14, 9 h 37'. The first and second satellites 
are seen in their places ; the situation of a third and fourth is 
pointed out. The first satellite is brighter than the second. 
X The first was 89^-° sf, and 16 0 2 6' from its greatest elon- 
gation; distance 574. The second was 8o° sp, and 7 0 56' 
from its greatest elongation ; distance 588. The superior 
brightness of the first therefore could not arise from its greater 
distance. The third and fourth supposed satellites had no 
subsequent observations. 
17 93, April 3, io h 33'. The first satellite is 30° nf ; the 
second is 8o° nf. 
J The first was 32|°nf; the second was 79 0 nf. 
1794, February 21, 8 h 24'. The first satellite is about 88° 
nf ; the second is about 86° nf. 
X The first was 89° nf ; the second 83° nf. 
1794, February 23, 8 h 24'. By a configuration the first 
satellite is at a great angle sp ; and its distance from the 
planet is greater than that of the second, which is at a much 
smaller angle sp. Several small stars are pointed out. 
X The first satellite was 84° sp ; distance 593. The second 
was 47^° sp ; distance 323. The stars were left in their 
places. 
Tt 2 
