Geology Reference
In-Depth Information
Ignoring radiative transfer, the energy equation for static equilibrium is
∇·
( k
T )
=−
H ,
(5.106)
where k is the thermal conductivity and H is the rate of heat production per unit
volume. Taking the curl of (5.104) yields
ρ ×∇
U
=
0,
(5.107)
showing that, in equilibrium, the surfaces of equal density coincide with equipo-
tentials, which by (5.104) are also isobaric surfaces. Equation (5.105) then implies
that the material on such surfaces has the same temperature, and is in the same ther-
modynamic state, provided that the composition and phase are assumed uniform,
and implies that we may take ρ, p , T , k and H all to be functions of U alone. Thus,
k T = k dT
dU U
=
f ( U )
U ,
(5.108)
where f ( U ) is a function of U . Substitution into (5.106) yields
2 U + f ( U )
∇·
( f ( U )
U )
= f ( U )
U ·∇ U
=− H ,
(5.109)
2 U from the governing
the prime indicating di
ff
erentiation. With replacement of
equation (5.5) for U , and with recognition of
U as the negative of the gravity
vector, (5.109) becomes
f ( U ) G ρ
2
2 f ( U )
2
Ω
+ g
=−
H .
(5.110)
In equilibrium, H depends on U alone, and therefore the left side of (5.110) must
depend only on U . From the analysis in Section 5.2, it is clear that, in general, g
2
cient f ( U ) must therefore
varies over any equipotential in a rotating Earth. Its coe
vanish, so f ( U ) is constant, giving
1
2
3 m ¯ρ/ρ
H
=
C ρ
,
(5.111)
the constant C being
3 f ( U )
¯ρ
GM
d 3 ,
C
=−
(5.112)
and ¯ρ being the mean density of the Earth,
3 M
d 3 .
¯ρ =
(5.113)
It is reasonable to expect the volume rate of heat generation to depend on the mass
density. Since m is only about 1
/
290 for the Earth, we can expect (5.111) to be
 
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