Models for the Crustal Structure of Io: Implications for Magma Dynamics

Details Models for the Crustal Structure of Io: Implications for Magma Dynamics Models for the Crustal Structure of Io: Implications for Magma Dynamics

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2274j&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2274

Physics

4

Scientific paper

We present a robust model for the crustal density structure of Io, which
we use to constrain magma dynamics with emphasis on the Prometheus
volcanic center. Preliminary results indicate that magma will pond at
shallow depths under a volatile layer.

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