Закономерности Кеплеровых движений. Бутиков Е.И. - 45 стр.

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m M
dm = (∆m/2π)
θ
P
r
2
+ R
2
2rR cos θ
P
dU(r) =
Gdm
r
2
+ R
2
2rR cos θ
=
Gm
2π
r
2
+ R
2
2rR cos θ
.
U(r)
dU(r)
θ 2π
U(r) =
Gm
r
1
2π
Z
2π
0
p
1 + (R/r)
2
2(R/r) cos θ
.
r À R
R/r ¿ 1
U(r)
Gm
r
1
2π
Z
2π
0
"
1
1
2
µ
R
r
2
+
R
r
cos θ +
3
2
µ
R
r
2
cos
2
θ
#
=
Gm
r
"
1 +
1
2
µ
R
r
2
1
2π
Z
2π
0
(3 cos
2
θ 1)
#
=
Gm
r
"
1 +
1
4
µ
R
r
2
#
.
U(r)
G(M m)/r
M m
r
U(r) =
GM
r
"
1 +
1
4
m
M
µ
R
r
2
#
=
gR
2
r
"
1 +
1
4
m
M
µ
R
r
2
#
.
GM gR
2
g
U(r)
r
F (r) =
dU(r)
dr
=
gR
2
r
2
"
1 +
3
4
m
M
µ
R
r
2
#
=
gR
2
r
2
"
1 + b
µ
R
r
2
#
.