320 Astronomical Observations at Barelly. [Junz, 
The longitude of Barelly from the mean of 8 occultations of stars 
in Oct. and Noy. last is 5 17 ™ 40 * 56 E. of Greenwich. 
By the mean of the 2 largest stars, Sagitarii and y Capricorn it is 5% 
17™ 39 § 68. 
The following emersions of Jupiter’s first Satellite were observed 
at Barelly in 1832. 
Difference from 
Mean time. Greenwich. Mean. 
hm. s. h 
October19th, 7 52 7 5 
26th, 9 47 48.9 5 
Nov... 4th, 6 12 48 5 18 0O 
5 
5 
‘ 17 35.7 
Ti th, S “Svar 17 24.7 ] 
Dec... 4th, 8 24 54 17 14 
Difference 
Srom Barelly. 
Re Themean ofthe observationsin Calcuttah. m.  s. h. m. s. 
ay (excluding the last) on the 19th Oct. 
D 1832, gives the emersion.. .. .. 8 28 3.5 0 35 56.5 
# oi | The mean of the three first on the 26th 
<j.09 ; 
ae Oct. gives the mean time of emer- 
2 ¢ | sion of Ist Satellite. .... .. ..10 28 27 0 35 38.1 
» Z |The observation on the 4th Nov. 6 48 38 0 35 50 
= The mean of the four observations on 
g the 11th Nov. gives the emersion 
g wf st Satellite... -.ccas i SRR 8 44 5.5 0O 35 49.8 
The difference of longitude deduced from Mercury’s 
RR it TS Sey eatin. eee secre eek tc 0 35 50.36 
The mean times of the observations of occultations of stars made at 
Barelly are, 
hm. s. 
October 2nd, No. 2276 Im. 10 21 23.9 
7th, No. 2814 Im. oo ais We 5 
28th, No. 2097 Im. 6 18 44.5 
29th, Osag.Im. 5 29 47 
Nov. Ist, y Capric. Im. 8 28 44.7 
Nov. érd, No. 2773 Im. 8 387 16 
» No. 2778 Im. 10 8 387.3 
bi Emer. 10 40 12.4 
