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Eruption Constraints for a Young Channelized Lava Flow, Marte Vallis, MarsThis study constrains flow rates for a specific channelized lava flow in Marte Vallis, Mars. We measured slope-gradient, channel width, and channel depth. Our results are similar to other recent studies which suggests similarities to long, terrestrial basaltic flow. Additional information is contained in the original extended abstract.
Document ID
20010045490
Document Type
Conference Paper
Authors
Therkelsen, J. P.
(Amherst Coll. MA United States)
Santiago, S. S.
(Arizona State Univ. Tempe, AZ United States)
Grosfils, E. B.
(Pomona Coll. Claremont, CA United States)
Sakimoto, S. E. H.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Mendelson, C. V.
(Beloit Coll. WI United States)
Bleacher, J. E.
(Arizona State Univ. Tempe, AZ United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2001
Publication Information
Publication: Lunar and Planetary Science XXXII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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