Hi,

I saw some comments on this board that relate to my abstract for the DPS
meeting.  I call
it my "Oceans 11" paper, since that's the number I come up with for
outerplanetary water-based oceans.  The BBC added some texture not
included in the abstract, at
http://news.bbc.co.uk/1/hi/sci/tech/2290005.stm.  

The general idea is that the small outerplanetary bodies like Pluto and
Triton (and not so small like Ganymede and Titan) are made up of ice and
rock.  The rock has sunk to the middle of the body.  Since the rock is
slightly radioactive, it gives off heat, which, for Titan, is on the
order of 100,000 megawatts.  If, at the interface of the ice and rock,
the
temperature is greater than the melting point of the ice (and opinions
vary on this temperature), then an ocean can be present.  

Long ago, the radioactivity rates were higher than today, so the
occurrence of oceans then was more likely than their occurrence now. 
Pluto and Triton were likely to have formed oceans in the past, and may
have
sufficient radioactivity today to maintain the oceans.  

For simplicity, clarity, and for maintaining a direct comparison among
the
many bodies studied, I ignored tidal and other heating sources.  Of
course, they
make oceans even more likely.  Charon, before it became synchronous with
Pluto, would have helped Pluto form the ocean.  

The chief unknown is the rate of radioactive heating.  I used a
present-day value based on values
for stoney meteorites.  Samples from the Moon taken by Apollo
astronauts, however, have twice this value, so there might be twice the
internal heating as I have assumed.  If so, oceans are quite common in
the outer solar system, the Kuiper belt, and even the Oort cloud.

Chris

p.s.  

I don't argue about the thickness of the crusts, but my calcs suggest
thicknesses of 66, 85 and 75 km for Europa, Callisto and Ganymede,
respectively.  These numbers are not authoritative, but might be
somewhat defensible.  

Christopher England
Technologist, New Millennium Program
Thermal and Propulsion Engineering Section
Jet Propulsion Laboratory
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