Arsia, Pavonis, and Ascraeus Mons, Mars: Rheologic Properties of Young Lava Flows

Details Arsia, Pavonis, and Ascraeus Mons, Mars: Rheologic Properties of Young Lava Flows Arsia, Pavonis, and Ascraeus Mons, Mars: Rheologic Properties of Young Lava Flows

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1277h&link_type=abstract

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

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We report on the rheologic properties of young lava flows on Arsia,
Pavonis, and Ascraeus Mons. We expand on our previous study in order to
investigate possible similarities and differences among the late-stage
lava flows of the Tharsis Montes.

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