of the Georgian planet. 327 
the second satellite. Some other small stars or supposed 
satellites are seen to the south at a good distance. 
J The first satellite was 79 0 nf ; the second was 81^° sf. 
The fourth proved to be a star. 
1794, March 28, 9 h 12'. The first satellite is 88° 31' np. 
9 h 1', the second is 82° 7' sf. 
J The first satellite was 87° np ; the second was 78° sf. 
1794, April 1, 9 h 14'. The first satellite i 83° 2' sp. 
9 h 23', the second is 70° 2 6' nf. 
J The first satellite was 87^ 0 sp; the second was 72 0 nf. 
1796, March 4, n h 10'. The Georgian planet is about 
13' of space preceding and 5 or 6 ' north of a nebula. An 
extensive configuration was made, but no satellites were 
noticed. 
J The nebula was No. 272 of the first class of my third 
catalogue. (See Phil. Trans, for 1802, page 505.) The first 
satellite was 42-§-° sp ; distance 158, invisible. The second 
was 87^ 0 np, distance 364, and after an interval of near two 
years might possibly be overlooked. The stars pointed out 
remained in their places. 
1796, March 5, i2 h 25'. The first satellite is 72 0 20' sp. 
io h 53'> 1 suspect a very small star between two of the let- 
tered stars of last night’s configuration which at the time it 
was made was not there. I had a pretty certain glimpse 
of it. 
J The first satellite was 75 0 sp. — io h 25', the second was 
72 0 np ; distance 1 23, invisible. By the configuration the sus- 
pected star was at a considerable distance, about 72 0 np. 
1796, March 9, 1 i h 35'. The first satellite is 70® 36' nf. 
1 i h 22', the second is 83° 3,5' sp. As the probability is that 
