Degree-1 Mantle Convection and the Origin of the Martian Hemispheric Dichotomy

Details Degree-1 Mantle Convection and the Origin of the Martian Hemispheric Dichotomy Degree-1 Mantle Convection and the Origin of the Martian Hemispheric Dichotomy

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1447r&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1447

Physics

Scientific paper

The hemispheric dichotomy on Mars may have been formed by degree-1
convection. 3D models with a layered viscosity structure can generate a
one-plume structure within 100 My, quickly enough to be associated with
the dichotomy.

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