( ) 
h - ; 
At 36* 01 Emerfion ef the greater Spot. 
9. 38. 26 Emerfion of the firft lefier Spot. 
9. 40. 2? Emerfion of the fecond lefier Spot. 
10. 204 04 The End of the Eclipfe. 
And he determined the time of the, total Datknefs 3'. 22' , 
or one Seeond lefs than by my Account. 
The Heavens were all the while very propitious to u$» 
and there was very little or no Wind, and not fo much as 
one Cloud interrupted our View from the Beginning to the 
End ; but no fooner was the Eclipfe over, but a great Bo- 
dy of Clouds hid the Sun for many Hours after. 
Thefe Observations having been made with all the Care 
we could, are not, ’eis hoped, far from the Truth. 
What we have received from other Places is as follows. 
The Reverend Mr, James Pound Re&or of Wanfted in 
M§ex and R. S. S. gives the following Account of the prin- 
cipal Phenomena obferved there ; he being furnilh’d with 
very curious Inftruments, and well skill’d in the Matter 
of Obfervation, and having rectified his Clock by feveral 
Altitudes of the Sun taken both before and after, viz. 
At 8; 6. 37 The Eclipfe firft perceived* 
9. 9. 28 The Total fmmerfion. 
9* 1 2. 48 The Emerfion. 
10. 20. 3 2 The juft End of the Eclipfe. 
f c. 3. 20 The Continuance of total Darknefs. 
The near Agreement of this Oblervation with our own 
(the Difference being only what is due to the Difference 
©four Meridians) makes us the lefs folicitous for what was 
noted at the Royal Ob [ervatory at Greenwich, from whence 
we can only learn that the Duration of Total Darknefs 
was 3', 1 1". 
The 
