4 Č ASTRONOMICAL. Aw» 
Remains the y'svifiblelongitude nearly, - 4 12 42-39 7 
Add the moon's parallax in longitude from. the 6. -]-21. 5, 3 
The fumis the »'s true long. according toobferv. 413 3 36,9 
"The true diff. of long. of © and » according to obferva. 6 1 gE 
: 6o 
375 
‘Let us now find the requifites for 7™ 11! 335" when tlie 
«eclipfe ended at Greenwich: 
Elements for computing the parallaxes, &c. at * r^ 33%! 
'The fun's longitude, i 4h 13?13'54^55 
The moon's ecliptic longitude, - 4 13 $3 55, 0 
The moon's latitude north, 28 40, 6 
"The fun's right afcenfion, ; 135 42 33 . 
The right afcenfion of the mii dene 243 35 55 
Angle pPZ, =o -THG 24 F 
‘Complement, | 63.35 55.2 
‘Side PZ as before, as alfo the p's horizontal parallax.® — X5 
From thefe clements are found ee 
‘The altitude of the noosgesinaal degree, - 20°11! 5" 
Angle PpZ, ! 326 12 38 
The longitude of the nonagefimal degree; kr 61238 
Angle 
_* As the moon was near her apogee, die horizontal parallax altered fo very itle 
in a few hours, that the fame may here be taken for the end, as for the beginning. 
NEL s 2E Rirdadagafertrpicipia. at the time of a folar eclipfe, al- 
lowancé fhould be made for the alteration of the horizontal parallax, between the 
beginning and end. 
