Methode zur Berechnung der absolut. Störungen der kl. Planeten. 127 
woraus 
N= 
C 0 ß(1.c) — £Ajß(2.c 
-£A s ß( 2. 
C 0 B(1.*)-£Ajß(2. 
+ -£ A 2 B{2. 
1 A 2 t1(0 
£A,ß(l. 
£Ajil(0 
und 
+ { C 0 .A(1 iC ) 
+ jiC 0 ß(2.c) 
+ j C 0 A(1.s) 
•+• ! 1 MM 
— ! 4' Aj A(1 .c) 
— jiVAj ß(2.c) 
— { £A, C(O.c) 
— j £ Aj A (1 .*) 
— S tVAj B(2.s) 
— ! 1 A t C(O.s) 
+ 1 MM 
+ } C 0 C(O.s) 
— ! C 0 C( o.c) 
■ £ Aj B('l 
- i A 2 il(1 
-tVA 2 B(2 
■ £ A 2 C(0 
- £ A 2 A ( 1 
A 2 ß(2 
t a 2 c (o 
i Aj A(1 
t Aj B (1 
t Aj ß(1 
■tV 
-i^CfO.c)) 
s)+H s C(0.s)) 1 ' 
s ) — r^i^’(o.s)i . 
c)-HA,C(0.c)j s " l(-, ' + ‘ ) 
.«)} COSe 
c)+ 1A 2 B(1 ,s)jcos( — y-t-2e) 
.s) j sin e 
•s)-iA 2 B('l x) j sin (— j/4-2e) 
.*) j cos 2e 
.«)) cos(— rj+3e) 
.«)] cos 
c) j sin 2e 
.c)J sin ( — r/4-3e) 
.c)j sin(?7+e) 
.s)+tA 2 ^4('I .c)} e 
•s)4-£A 2 ß(1 .c) j e cos ?] 
.c)4-£A 2 ß(1 .*) | e sin y 
N- f{ (g?) de = | -2C 0 //( I .c) 4-^A 2 77(0. s) j cos * 
4- [ iAj/7( I x) — £A 2 77(1 .*) i cos 2e 
4 - ) — 26’ 0 77(l.s) — -f-A, 77(0. s)j sine 
4- j £Aj/7(1 .$) 4- 1 A 2 /7( l x)j sin 2e 
4- \ o 6 o 77(0.s) 4 -£Aj 77 (1 .$) — £A 2 /Z(1 .c) j e 
hervorgeht. Für die übrigen Producte ist jetzt 
= — A, sin e 4- A 2 cos e 
4- e//(0.s) 4- {77(1 .c) — 7/(0.c)jsin e — { 77(1 .«) — //(O.s)jcos e 
— 7/(0. s)e sine — 77(0. c)e cose 
^ A, 4- Aj cos e 4- A 2 si n e 
4-~f-77(0.s)e 4-77(0.s)e cose — 77(0.c)e sin e 
v 4- - = ( C’ 0 4- K 4- — ) — £ Aj cos e — 4 A 2 sin e 
— £77(1 .c) cose — £77(1 .s) sin e 
— £ 77(0. s)e cose 4-- J-77(0.c)e sin e 
2 r = 2C 0 — A, cos e — A 2 sin e 
4- 77(1 x) cose 4- 77(1 .s)sin e 
4- c77 (O.s) e 4-77f0.s)e cos e — 77(0.c)e sin e 
