Volcanic Spreading at Olympus Mons: New Models, with Implications for Martian Volcanic Edifice Structures and the Distribution of Phyllosian Sediments

Details Volcanic Spreading at Olympus Mons: New Models, with Implications for Martian Volcanic Edifice Structures and the Distribution of Phyllosian Sediments Volcanic Spreading at Olympus Mons: New Models, with Implications for Martian Volcanic Edifice Structures and the Distribution of Phyllosian Sediments

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2304m&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

The flank topography and tectonics of Olympus Mons are best explained by
volcanic spreading upon basal sediments thickening with distance from
Tharsis, if those sediments are clays from the proposed Phyllosian
epoch.

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