3 2 9 
of the Georgian planet. 
1796, April 5, io h 48'. The first and second satellites are 
apparently in opposition, the same wire covers them both and 
the planet. There is no star in the line of the transverse 
that can be taken for a satellite: the night being beautiful,, 
I examined that line with 300 at a distance, and with 600 
within the orbit of the two satellites. 
X The first satellite was 74y° nf ; the second was 8if 0 sp. 
1 797, March 15, 9 h 44'. The first and second satellites are 
not far from their opposition ; by the configuration they are 
short of it. 
J The first was 78J 0 sp ; the second was 8i£° nf. 
1797, March 17, 9 h 51'. The first and second satellites 
are both invisible; the night is very beautiful and I have a 
field bar to hide the planet ; but notwithstanding this, I can- 
not see either of the satellites ; many stars are pointed out. 
J The first was 6g^° sf ; distance 110, invisible. The 
second was 76° np; distance 126, invisible. The stars had 
no subsequent observation. 
' 1797, March 21, io b g'. The first satellite is not visible ; 
the second is nearly at its greatest elongation, it is about 70° 
south preceding ; many stars are pointed out. 
X The first satellite was BS-^ 0 np ; distance 240, invisible; 
the second was 7 g\° sp; distance 588. The stars remained. 
1797, March 23, io h 28k With 320, 1 see neither of the 
satellites. io h 32', having just been told where the second 
should be, I perceived it in its place ; with 600 I see it very 
well ; many stars are pointed out. 
X The first satellite was 76° sp; distance 518 ; it does not 
appear why it could not be seen. The second was 88° sp ; 
distance 298. The stars remained. 
U u 
MDCCCXV. 
