œ ASTRONOMICAL ARE AM 
(P 389920280 betes | 
€ 9 9390986 ^. 
x nearly 2807", 4 bog 4483011 
sono m 46! 4a 8 
“ps tue lat. ge? 17 N 
jp. viz. $6 vi at. 13. go S Sine 7 040588, ag 
de ca PD 32933995. 1% 
“SPS yeh. “8255 Voshine & 1. (9: 2855507 
fait, pm vy sl sse fs 
x nearly 464 47; «€ d ronds A 
erg od. Bu 
= Pee e $1, 2 Y'sparallaxinlat. from o |. 
Sine ae i p222'12^ S'gggéPios 72 
E Sine 3 | 52 23 17 9 8988143 — 
Soren ipes 5 = 884% 5 2 9466978 — 
: Her augmented or r vifible $n 
pee j 808,82 9487629 
= 14! 48", 8 
LI 
“By thefe refults it appears that the foregoing paue: find 
the parallaxes and augmented femi-diameter of the moon to 7 4 
‘great exactnefs. 
Let pe iol die eas dence of longitude between 
the center of the fun and moon, at Greenwich, at 5^ 29‘ 57^, 
when the eclipfe begun there. Plate I, Fig. IV. - 
"The 
