Scale of volcanic activity.
I am wondering if there is a simple computation (*) (using the
mass, age, internal radioactive heating, magma viscosity, ...) that
can give the order of magnitude of volcanic activity (measured for
example by the volume of crust produced per year, thermal energy loss
through eruptive activity,...). I know that astronomers do similar
computations for stars, trying to estimate brightness, neutrino flux,
lifetime, composition...
(*) This computation could probably apply to any planet.
Jacques D. Rutschmann
Dear Jacques,
I mentioned your question to Chuck Wood. Since Chuck spends the better
part of most days thinking of space (he's Chair of the Space Studies
Department), he promptly reminded me that modeling stars (ideal gases,
homogeneous) is a lot easier then modeling the Earth (solid, liquids,
gases; non-homogenous in composition, distribution in radioactive
elements, and viscosity).
With that said lets do a simple computation. For 1 calorie of heat
extracted from the mantle 0.01 g of melt is generated. Assuming a
density of 3.2 gm/cc and a volume of 125 cubic km/year for new oceanic
plate created at mid-ocean ridges (and probably ten other things I didn't
even think of), about 5E12 watts of energy are transferred from the
mantle to the surface by mid-ocean ridge volcanism.
So, I came up with this number and wondered if it means anything (does it
say anything about the amount of thermal energy loss through eruptive
activity). I found some interesting values for energy flow in the Earth.
About 20-40 watts of energy are conducted from Earth's interior to
the surface. So my value is not too far off and suggests volcanism plays
a significant role in cooling the interior of the Earth. U.S. Energy
consumption (in 1980) was 2.5E12 watts, roughly half the energy released
by heat transfer at mid-ocean ridges.
Steve Mattox, University of North Dakota
Source of Information:
Harte, J., 1988, Consider a spherical cow, a course in environmental
problem solving: University Science Books, Mill Valley, California, 283 p.