HR: 0800h
AN: P51B-0931 [Abstracts]
TI: Towards a Power Balance for Earth's Interior
AU: * Anderson, O L
EM: ola@ess.ucla.edu
AF: Institute of Geophysics and Planetary Physics and Department of Earth and Space Sciences, University of
California, Los Angeles, 595 Charles E. Young Dr. E, Los Angeles, CA 90095-1567
United States
AB:
The purpose of this presentation is to enumerate
and describe the major power mechanisms
and find a power balance for Earth's interior that
compares favorably with a well-accepted measured value.
The power leaving Earth's interior is the total
power produced by sources (such as radiogenic activity)
modified by the total power of passive
mechanisms (such as plumes) that transfer power from one part of Earth
to another. There are five power sources: (1)~The radiogenic
power of Earth, found to be 31.2~TW (2.1~TW in the core and 8.2~TW
in the continental crust); (2)~gravity release
due to thermal contraction
as the temperature declines; (3)~internal
friction due to mantle convection; (4)~heat of
crystallization released as the inner core grows;
(5)~power associated with convection
arising as fractionation proceeds on
the ICB boundary.
Several passive transport mechanisms
convey power from one site to another in
Earth by means of a negative thermal gradient
dT/dr, where r is the radius
measured to the center.
The value of heat flux flowing outward is controlled
by the Fourier law of conductive heat flow
or by conductive heat flow (found in D'',
the mantle, the lithosphere, and the outer core).
Convective heat flow is found in plumes and hydrothermal
cooling of the lithosphere.
In the circulating system of mantle convection, some mechanisms
have a compensating negative counterpart. An example
is the melting of the mantle to produce liquid basalt
at the ridge axis, which requires energy. But subsequent
solidification cancels
the effect of melting in the power budget
because it releases the same energy.
Our analysis consists of finding and evaluating sources
and transfer mechanisms.
The net power leaving the system
is found to be 40.2± 5 TW, in substantial
agreement with the value of Pollack et al. (1993),
who reported the average heat flow leaving Earth
as 87 ± 2.0m̅W m-2
(or 44.2 ± 1 TW).
DE: 5418 Heat flow
DE: 5430 Interiors (8147)
DE: 8147 Planetary interiors (5430, 5724, 6024)
SC: Planetary Sciences [P]
MN: Fall Meeting 2005