On Convection in Ice I Shells of Outer Solar System Bodies--Application to Callisto and Titan

Details On Convection in Ice I Shells of Outer Solar System Bodies--Application to Callisto and Titan On Convection in Ice I Shells of Outer Solar System Bodies--Application to Callisto and Titan

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2387m&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2387

Computer Science

Scientific paper

Convection in Callisto's floating ice I shell is possible for reasonable
grain sizes. Diffusion creep is the key. Not only possible, but probably
required throughout much of Solar System history. For Titan, it depends
on grain size and composition.

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