The Formation History of Olympus Mons from Paleo-Topography

Details The Formation History of Olympus Mons from Paleo-Topography The Formation History of Olympus Mons from Paleo-Topography

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2202j&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2202

Physics

1

Scientific paper

We use lava flows on the flanks of the flexural trough surrounding
Olympus Mons to reconstruct the history of volcanic loading and flexure.
We constrain the eruption history and rates using paleo-topography,
flexural modeling, and crater counting.

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