Slow Secular Cooling and Long Lived Volcanism on Mars, Explained

Details Slow Secular Cooling and Long Lived Volcanism on Mars, Explained Slow Secular Cooling and Long Lived Volcanism on Mars, Explained

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1285s&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1285

Computer Science

Scientific paper

We use thermo-chemical convection models including partial melting to
demonstrate that focussed persistent volcanism can occur on Mars. Our
results provide an explanation for the existence and longevity of a
single giant volcanic complex on Mars.

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