Evaluation of the Orogenic Belt Hypothesis for the Formation of the Thaumasia Highlands, Mars

Details Evaluation of the Orogenic Belt Hypothesis for the Formation of the Thaumasia Highlands, Mars Evaluation of the Orogenic Belt Hypothesis for the Formation of the Thaumasia Highlands, Mars

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1069n&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

The orogenic belt hypothesis for the formation of the Thaumasia
Highlands is tested using critical taper wedge mechanics. We find that
conditions required for their formation as an orogenic belt are
improbable for Mars.

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