The Formation of Hrad Vallis, Mars, and Its Associated Deposits by an Explosive Sill-Cryosphere Interaction

Details The Formation of Hrad Vallis, Mars, and Its Associated Deposits by an Explosive Sill-Cryosphere Interaction The Formation of Hrad Vallis, Mars, and Its Associated Deposits by an Explosive Sill-Cryosphere Interaction

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1273w&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1273

Physics

1

Scientific paper

We show that the morphology of the Hrad Vallis depression and its
associated deposits can be explained as the result of a violent
phreato-magmatic explosion when a 30-100 m thick sill intruded at
shallow (~400 m) depth into volatile-rich crust.

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