The Stress State of a Growing Lunar Crust: Implications of the Cooling of a Magma Ocean

Details The Stress State of a Growing Lunar Crust: Implications of the Cooling of a Magma Ocean The Stress State of a Growing Lunar Crust: Implications of the Cooling of a Magma Ocean

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1192s&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1192

Computer Science

2

Scientific paper

We address the early thermo-mechanical evolution of a lunar crust
forming from a magma ocean to assess conditions under which early
volcanism may have occurred. Potentially large compressive stresses may
have been temporally and spatially common.

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