[ 4^3 1 
Difference of Right Afcenfion between the n ’s Limb and * ’$♦ 
1 Time per Clock. 
Time per 
Clock. 
Sept. 
s—s; 
)’s2dlimbpa(Tedli 
re wires vertical t 
0 the equator, v 
6 Pifces parted 
le fame vertical 
/ires. 
h > " 
h ' " 
21 4 14+ 
26 
3 8 
49 
5 1 
'| The 4 would 
| not follow 
l through the 
f field of the 
J telefcope. 
if— 20 
20 24 34 
24 47 + 
2 4 59i 
25 12— 
20 26 13 
26 25I 
37— 
26 49 
20 31 54— 
32 6 
32 i8§ 
20 33 I2| 
24— 
33 36 
37 27— 
37 3 8 i 
57 5' 1 ! 
3 8 3 1 ' 
42! 
3 8 54+ 
10 42 51 — 
43 4 
J 7 
43 53 
44 5i 
2 9 
43 4i— 
J 7 
44 5 + 
20 50 55— 
5i 7i 
5 1 2 3 i 
5i 35§ 
\ 
58 29 
58 42 
58 56+ 
59 8 
20 59 21 
5 8 37 
5 8 50 
59 3 
59 Hi 
10 59 26 
21 1 — 
21 2 
2 t 3 35 
the 2"after 
the ]) ’slimb. 
The ]) ’slimb and 
4 equal in A. R. 
as near as could be 
judged. 
The J) followed 
the 4J5" in time. 
21 7 50 
21 11 
Clouds 
Clear 
Sept. 
? 20 
1 6 Pi fees parted 
the wires vertical 
to the equator. 
']) ’s ad limb paf- 
fed the lame 
wires. 
22 23 41 
54 
24 6-f 
17 + 
24 29l 
30 47 
31 1 — 
13 
2 5 
3 1 37 
43 19! 
33 + 
44 
22 43 56 
22 51 32-f 
45i 
58 
52 9 + 
52 2lf 
56- 
9— 
22-f 
33 + 
45 + 
16 — 
29 
23 
2 
3 
3 
15 
22 27 14 
27 + 
40 + 
5 2 
28 4 + 
34 4° 
53 
35 6 + 
18 
35 30 + 
47 42 
54f 
48 6f 
48 19-}- 
5 6 r 5 
28 
41— 
5 2 f 
57 5+ 
8 7 — 
20 
3 2 
44i 
8 57 
20 55 
21 9 — 
>3 
J above. 
The Star was to move along the equatorial 
wire in all thefe obfervations, and I look 
upon the whole to be very good ; particu- 
larly thofe after the occupation, as the dif- 
ference of declination of the ]) ’s center and 
Star was by eftimation not more than 4 or 
nor even fo much at the laA obferva* 
tions. 
Q.q q 2 
