22 
©’s long. from the + aati 2° 
©’s horizontal para 
©’s semidiameter —Teraiaton 3” 5 
©’s horary motion 
Avge obliquity of the ecliptic 
d’s rom the apparent equinox) 
)’s horary motion 2 the® in Jone: 
ral 
D’sp arallax—©’ sp 
Parallax in longitude ()}—© ) 
Parrallax in latitude ¢ ») —o) 
Observations on the eclipse of the sun, June 16, 1806. 
Beginning of |Beginning of to-| End of total End of the 
eclipse. tal darkness arkness eclipse. 
St Ft yy So. 7 0. 4a Soo 7 
2°24 41° 2 3/2°24-44°11* 012°24°44°22° 4/2°24°47°34° 6 
8 5 a ¥ 8° 8: 
15°42° 5 15:42 § 15°42° § 15°42" 5 
2°23°15 2.23°15 2°23°15 2°23°15 
23°27°50 23°27°50 23°27°50 23°27°50 
2°23°49-28° 8)2°24°37°47° 712°24°40°43° 812°25°29°58° 3 
24°34" 4 20° 6° 5 19°50° 3 15°17. 3 
60° 9: 0 60°10" 4 60°10" 5 60°12" 0 
16°39" 7 16°41° 4 16°41" 4 16°41° 7 
36*39'92 36°41°77 36°41°89 36°43°72 
S232 3°23°62 3°23'62 3'23°95 
34° 16°77 34°18°62 34°18°7 34°20: 57 
60° 0 5 60° 1: 9 60° 2° 0 ie ee 
19°44 2) +4 553° 1) OS" OF Of =e 9°57" 9 
—22°27 9] ~—20* O 2} — 55° uz oo” 5 
Now if the latitude of the moon by the rr be aaopaied to be 
the €eliptic: conjunction. at, Salem_wi 
11h. $7’ 20:3 by the mean of all the ono “This will be i in- 
creased only 04, by decreasing the latitude 6-9, which appears to be 
necessary from the observations at Rutland, Pawlet, &c. as given by. 
Doctor Williams and others. _ 
‘I shall continue this subject in another memoir. 
correct, the mean time of 
nS epee Par OR Paes ele 
