Mystery of Callisto

Details Mystery of Callisto Mystery of Callisto

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..923m&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 923.

Computer Science

Callisto, Satellite Surfaces, Galileo Spacecraft, Polymorphism, Ice

Scientific paper

New undifferentiated interior models have been calculated for Callisto using the ICYMOON code of Mueller and McKinnon (1988), which can handle one-, two-, or three-layer icy satellites. A typical temperature profile through Callisto is conductive near the surface and becomes adiabatic in the convective region. Callisto is significantly self-compressed due to the polymorphism of the ice phase.

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