The Thick-Shell Model of Europa's Geology: Implications for Crustal Processes

Details The Thick-Shell Model of Europa's Geology: Implications for Crustal Processes The Thick-Shell Model of Europa's Geology: Implications for Crustal Processes

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1866p&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1866

Physics

6

Scientific paper

The gamut of Europa's endogenic surface features can be accounted for by
tidal deformation coupled with the buoyant rise and partial melting of
warm ice within a relatively thick (nominally ~20 to 30 km) icy shell
above a liquid water ocean.

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