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so that
V≈
ρ(
r
0
)
δ
s
ρ
d
δ
r
0
dr
0
dS
=
ρ(
r
0
)
∂
R
∂
r
0
R
2
sinθ
d
θ
d
λ
dr
0
,
(5.148)
after substitution for δ
s
/δ
r
0
from (5.146). ρ(
r
0
) is to be interpreted as the density
on the equipotential with mean radius
r
0
. Similarly, since the intensity of gravity is
inversely proportional to the orthometric separation of the equipotentials,
≈
δ
U
i
=
δ
U
i
δ
r
0
δ
r
0
g
dS
δ
s
dS
δ
s
dS
1
(1/
R
2
) (∂
R
/∂θ
)
2
∂
R
/∂
r
0
+
dU
i
dr
0
R
2
sinθ
d
θ
d
λ
.
=
(5.149)
Together with the addition theorem (B.9),
n
1)
k
P
n
(cosθ)
e
ik
λ
P
−
n
(cosθ
)
e
−
ik
λ
P
n
(cos
Θ
)
=
(
−
,
(5.150)
k
=−
n
(5.148) and (5.149) can be used to reduce (5.138), including (5.140), to the single
scheme
4π
GP
n
(cosθ)
d
r
0
ρ(
r
0
)
π
R
n
−
1
∂
R
1
∂
r
0
P
n
(cosθ
)sinθ
d
θ
dr
0
0
2
P
n
(cosθ)
π
0
P
n
(cosθ
)sinθ
R
r
0
dr
(
r
)
n
−
1
d
θ
+
2
Ω
dr
0
P
n
(cosθ)
π
(1/
R
2
) (∂
R
/∂θ
)
2
∂
R
/∂
r
0
dU
i
1
R
n
−
1
1
+
P
n
(cosθ
)sinθ
d
θ
+
0
2
GM
2
r
0
,
n
⎩
2
−
3
Ω
=−
1,
2
U
i
2
r
0
,
−
+Ω
n
=
0,
=
(5.151)
2
P
2
(cosθ),
n
(2/3)
Ω
=
2,
0,
n
=
1,3,4,5,
···
.
In arriving at the relations (5.151), the following should be noted: all the terms in
the summation in the addition theorem for
k
0 vanish on integration over azimuth;
and the second integral on the left of (5.138) over the volume
0
involves
integration over radius from
r
0
to
R
, with
R
a function of θ
, so the integration over
radius is to be completed before the integration over θ
.
V
−V
i
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