A New Hypothesis for the Origin of Mass Movements on Callisto

Details A New Hypothesis for the Origin of Mass Movements on Callisto A New Hypothesis for the Origin of Mass Movements on Callisto

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2901w&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2901

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Scientific paper

We will describe a new hypothesis for the origin of the large lobate
mass movements seen on Callisto but not other Galilean satellites. The
mechanism involves near-surface condensation of CO_2 vapor driven upward
by the geothermal gradient.

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