Satellites of the Planet Saturn. 4 ^/ 
Sept, 25. 22 36. The 6th almoft * projeftion f. the edge of 
the R. 
23 42. The 6th fat. very nearly 1 projeaion f. R, (R). 
23 52. The 6th fat. is much larger than the ;th. 
Oa. 1 2. From 22 h. 6' to 1 h. 8' (S). 
0 58. The feventhfat. extremely fmall upon the point of the 
preceding projeaion, and a little towards the fouth. 
1 20. The diftance of the feventh increafes. The fatellite 
feems to be clear of the projeaion ; but I can fee no divifion 
yet, its whole dia. feems to be to the fouth ^ I fee it full aft, 
well as I faw the 6th, or rather better (T), 
1 35. The feventh is clear of the projeaion. 
Oa. 1 5. 20 47. The 6th fat, 1 dia. of ^ p. the body. 
21 34. The 6th about | of the projeaion p. the edge of R. 
or very near 1 dia. of i? p. the body ; juft ft. the 3d , it is in the 
line of theR. (V). 
22 25. The 6th fat. will be in conjunction with the 3d in a 
very fhort time, the 3d being ftill a little p. 
22 39. The conjunaion is fo complete now, that I have loft 
the 6th. The 3d, however, appears to be a little lengthened 
out towards the fouth. Diftance of the conjoined fatellites 
(R) 1 1 h. 12' 52". 67°, 7. 
(S) There were five obfervations made upon the 6th fatellite, but they belong 
to the 7th. There were alfo three obfervations made upon the 7th which belong 
to the 6th, and are here given ; we are to obferve, that the revolution of the 7th 
was not yet afcertained, and that, confequently, a miftake of one new fatellite 
for another could eafily be made. 
(T) nh. 43^53^. 220°, 9. The calculation of its place {hews plainly 
that it was the 6th; and the remark in this obfervation of its being brighter than 
the other fatellite perfe&ly agrees with the calculation. 
(V) 7 h. 46' 43". 246°, O. 
P p p 2 
barely 
