48 ASTRONOMICAL anD 
latitude, as. given by them, the correction of which may ie 
found, in the manner following :- 
The y's longitude at the beginning, per tables, 3*3? 6/3240 
‘The »'s parallax in longitude from @ me 30 47, | 
| | sey 
The »'s longitude at the end per tables, 3 4 12 3 
"The »'s parallax in longitude from © — 36 
: 3-3 3$ 
Subtract | 3 2 35 
Difference | 1.0 23 I 
Subtract o's motion during the eclipfe, 4 10, % 
Remains p's vifible motion from © per tables, — 55 52; 
3352, 9 
The »'s vifi. Ja. fono by ealeslation st egg, “4 
| At the end, EET AC 
j Ee x: (T vifible motion in. latitude from t the o,* 
“ie pice 5s Ge. = let BoC be a portion of di ec $2 
335 2 the moon's vifible motion from the (un, during the 
| eclipfe 
> k D ea i-is difis-from Jur horary motion and parallaxtt- 
poe is not affected by the fmall error in the latitude given by the tables« - 
4 Sec ute, page 7, 
