L 
there was feme Time loft in direding it towards the 
Sun; and when I got the Image in a due Pofition, there 
was left than n Digits eclipfed; and Ifufped that it 
never amounted to full 1 1 Digits. I had no Micro- 
meter. - 
After taking fome more Digits, I went with Sir 
John Clerk to a neighbouring Houfe, to obferve the 
End of the Eclipfe, being afraid we fhould not be 
able to fee it from the College. By a„Signal that was 
made to the Perfon who attended the Clock, (two Se- 
conds being fubduded, that were loft in making the 
Signal) the End . was at 4 Ho. 44 Min, yi Sec. The 
Wind blew hard at this time, Co that the Telefcope 
.could, not be kept very fteady, and there was fome 
Undulation on the Circumference of the Sun 5 but I 
cannot think that the Error of this Obfervation can 
exceed three or four Seconds, the Circumference of 
the Sun appearing to me complete at that Inftant. 
I fhall now fubjoin the Observations that were made 
in the Caftle and College in one View, by which you 
will fee that they agree precifely as to the Continu- 
ance of the annular Appearance, a Coincidence that 
copld not have been expeded 5 but fo it is, according 
to the Numbers that were given me immediately after 
the Eclipfe by thofe who attended the Clocks. 
The 
