Plains Volcanism on Mars Revisited: The Topography and Morphology of Low Shields and Related Landforms

Details Plains Volcanism on Mars Revisited: The Topography and Morphology of Low Shields and Related Landforms Plains Volcanism on Mars Revisited: The Topography and Morphology of Low Shields and Related Landforms

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3287h&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3287

Physics

Scientific paper

The morphology of landforms associated with plains volcanism on Mars is
fully consistent with basaltic volcanism on Earth. The flank slopes of
low shields are among the lowest in the solar system, indicating a very
low viscosity of the lavas.

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