of the Georgian planet. 325 
is a proof of the great attention that was paid to ascer- 
tain the nature of supposed satellites. The small stars 
remained. 
1794, March 7, n h 18'.- I cannot perceive the first satel- 
lite. io h 57', the second is nearer the planet than it was the 
last time I saw it. Small stars are pointed out. 
J The first was 63° sf ; distance 320, invisible. The se- 
cond was 87f° np. There is no subsequent observation of the 
small stars. 
1794. March 17, 7 h 38'. I can see neither of the two 
satellites. 
J The first was 41 0 nf ; distance 292, invisible. The se- 
cond was 383" 0 nf; distance 285, invisible. 
1794, March 21, n h 53'. I cannot see the first satellite. 
I looked at several different hours for it. io h 53', the second 
satellite is 88° 8' np. 9 h 19', the place of a small suspected 
star is pointed out, but it cannot be verified with 460 and 
600. 
J The first satellite was 27° sp ; distance 243, invisible. 
The second was 81^° np. The suspected star was seen in 
its place the following night. 
1794, March 22, 8 h 47'. There is no mention of the first 
satellite ; the second is 6'T 46' np. 
J The first was 66^° sp, and its distance being 480, it must 
have been seen and taken for a star. The second satellite 
was6o^°np; distance 311. 
1794, March 23, 8 h 32'. The first satellite is one of two 
small stars that are south of the planet ; it is the preceding 
and largest of the the two. 8 h 42', the second satellite is not 
visible. 
