of the Georgian planet . 339 
There are so many small stars that it is next to impossible to 
look for the additional satellites. 
J The first satellite was 79 0 nf ; distance 546. The second 
at 8 h 45' was 77-S- 0 nf ; distance 453. 
1798, April 8, io h 19'. There is no satellite visible between 
the second and the planet ; the second satellite is north fol- 
lowing, at a greater distance from the planet than last night. 
There is a very small star at a little more than twice the dis- 
tance of the second satellite north following. 
J The first satellite was 8oj° nf; distance 239 ; invisible. 
The second was 78° nf ; distance 576. The small star re- 
mained in its place. 
1798, April 9, 9 h 34'. I cannot see the first satellite. The 
second is at a distance north following, rather farther from 
the planet than last night. With 480 and 600, there is no 
satellite between the second and the planet. 
J The first was 74-j 0 sp; distance 171; invisible. The 
second was 79 0 nf; distance 578. 
1798, April 11, 9 h 8'. The first satellite is south preceding 
at a considerable distance ; but not at its greatest elongation. 
I cannot see the second satellite. I suspect a very small 
star in the line of the north following greatest elongation, a 
little farther from the planet than the first satellite. With 
480 I cannot verify the suspicion. 
J The first satellite was 78^- 0 sp ; distance 587. The se- 
cond was 8o^° nf ; distance 247 ; invisible. This satellite 
could hardly be the suspected star, as it was but at little more 
than half the distance of the first satellite from the planet. 
1798, April 12, 9 h 54'. I cannot see the first satellite, nor 
the second. With 480 there is no satellite either new or old 
X x 2 
