C A P V T II.

- — ^ — i5 8", 3 fin. p — <5

+ 39 o - // , 9-fi n ‘ 2 / ) +

+ 27 ,/ ,o.fin.4p —

+ 6, i. fin.(p-b-) +

+ i 8,2.fin (2p+2<?) ++ 23, i.fin.(p-#) ~

+ 3 / .i8,8.fin.(2p-2^) -

— 3 19,9 fm.(2/H?) +—i*. 1 6 *. 1 5,7. fin (2p-§) —

-+ 33,2+m.(4p-2^) —

— i7,9.5m.(2p-3-) +

— i'- 8",l.fin.(4p-§) +

6c>3

17^ 2i w } o. fin. ^

12. 57, 8. (in. 2 q37. 1. fin. 3 q

1i' 2z",o.fiu.k23, 3. fin. (2p-K)2. 39,C.fin (2p-;)

1. 48, 2. fin (y+f)

2. 23,7 fin.(--r)

1 x, 0+111.(27-/)

2<5,8.fin.(2p-y+;)20,3 fin.(2p+^-/)3 ' i8,3-fin.(2p- ? -01 l,8.lm.(2p-2§ /)

+ i 1 . 1,7.fin (2p-2r)

- 1. 27,8+111. (f-sr)

§. 562.

Perfpicuum autem eft hanc formulam nondumconuenire cum angulo noftro <P, fed illi infuper ad-jici debere illam particulam, quae ab Aflronomis, vo-cari solet redudlio ad eclipticam ita vt pofita hacredu&ione ~ g, tum demum habeamus ^4^

verum hanc ipsam rednftionem Celeb. Clairaut 1e-

G g g g 2 quen-