Geology Reference
In-Depth Information
the Earth ( r
=
d ), this expression becomes
2 d 3 1
3 I 33 P 2 (cosθ)
GM
d
3 G
1
3 I 22
2
V
=−
3 I 11
+
2
2
3 I 13 P 2 (cosθ)cosφ +
3 I 23 P 2 (cosθ)sinφ
(4.52)
+
1
6 ( I 11
1
I 22 ) P 2 (cosθ)cos2φ
3 I 12 P 2 (cosθ) sin 2φ
+··· .
Since the solid spherical harmonics in expressions (4.41) and (4.52) are linearly
independent, equating V 2 to k 2 U 2 following equation (4.34) gives five equations in
the six components of the inertia tensor. A sixth equation is
Tr( I )
=
I 11
+
I 22
+
I 33 .
(4.53)
Solution of these equations for the components of the inertia tensor yields
Tr( I )
k 2 d 5
3 G ω i ω j
k 2 d 5
2
1
3
ω
i
I ij
=
+
δ
j .
(4.54)
3 G
2 d 2
The termω
/3 in the deforming potential (4.41) will cause a purely radial expan-
sion, contributing only equal amounts to I 11 , I 22 , I 33 , thus altering only Tr( I )
(Rochester and Smylie, 1974). The contributions to the inertia tensor, r ij , caused by
deformation under the changed centrifugal force, neglecting squares and products
of the small quantities m 1 , m 2 , m 3 ,arethen
2 k 2 d 5
9 G Ω
1
3 Tr( R )
2 m 3
r 11
=
2 k 2 d 5
9 G Ω
1
3 Tr( R )
2 m 3
(4.55)
r 22 =
4 k 2 d 5
9 G Ω
1
3 Tr( R )
2 m 3 ,
r 33
=
+
where Tr( R )
= r 11 + r 22 + r 33 is the contribution to the trace of
the inertia
tensor, and
k 2 d 5
3 G Ω
k 2 d 5
3 G Ω
2 m 2 , r 13
2 m 1 .
r 12
=
0, r 23
=
=
(4.56)
Thus, the complex phasor,
k 2 d 5
3 G Ω
2 m ,
r
=
r 13
+
ir 23
=
(4.57)
 
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