483]
EQUATIONS IN THE LUNAR THEORY.
539
Q 1 = km 2 (|- + f cos 2D),
Q. 2 = km? {3^ sin 2D + pi (| + f cos 2D)},
Q s = km 2 {— Sv 2 sin 2D — 3wj 2 cos 2D
4- PtV x . 3 sin 2D
+ PÁ2+ f cos 2D)},
&c.
P 1 —jm 2 (— f sin 2D),
Po =jm 2 (— 3v x cos D — 3p x sin 2D),
P 3 =jm? {— 3v 2 cos 2D + 3y x 2 sin 2D
— QpiV x cos 2D
+ (2/o 3 + /Op). - f sin 2D},
&c.
In particular attending to the values of P 15 Q x the equations for p x , v x are in their
original form
it d ir^ d iD hm ^ + §™ m -
cl (dv
dt \dt
+ 2 p ;
—jm 2 ( — I sin 2D),
whence in the transformed form they are
and
dv x
dt
d~pi
dt 2
3jm?
4 (1 — m)
+ 2p x = Hj 4- t jdj ' "' :z\ cos 2D,
+ Pi = 2fli + km?{\ + f cos 2D) + cos 2D.
dv,
Thus the constant term of p x is 2Q. x + \km?, giving in —^ a constant term — 3ilj — km 2
this must vanish, or we have ilq = — km 2 ; and the equations thus become
~ +2= — 1 km 2 + cos 2D,
4 (1 — m)
+ pi = — £&m 2 + km 2 + cos 2D,
and then completing the integration
— #&m 2
Pi = ~i km 2 +
+
— fjm 2
3 — 8m + 4m 2 (1 — m) (3 — 8m + 4m 2 ) j
cos 2D,
Vi =
\km?
+
§ jm 2 (7 - 8m + 4m 2 ) j gin w
((1 — m) (3 — 8m + 4m 2 ) (1 — m) 2 (3 — 8m + 4m 2 ) j
which are the accurate values of p x and v x .
Expanding as far as m 6 we have
p 1 = k(— ^ m?) + cos 2D { k (— m? — f m 3 — - 2 ^- m 4 — m 5 — m 6 )
+i (— | m 2 — ^ m? — f| m 4 — Afi 5- m5 ~ tW- w 6 )},
which for j = & is =fc(- m 2 -J^m 3 -^m 4 - ^ m 5 - ^ m 6 ) ,
68—2