Tharsis Formation from Density Driven Thermo-Chemical Plumes During Planetary Differentiation

Details Tharsis Formation from Density Driven Thermo-Chemical Plumes During Planetary Differentiation Tharsis Formation from Density Driven Thermo-Chemical Plumes During Planetary Differentiation

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2522f&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2522

Physics

Scientific paper

We propose a new model for Tharsis formation as a thermo-chemical plume
that forms during differentiation processes on Mars. Fluid experiments
using liquid gallium suggest a buoyant anomaly may postdate a
Borealis-sized impact and core-forming event.

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