Testing the Late-Stage Outflow Channel Origin Hypothesis: Investigating Both Water Erosion and Lava Erosion Origins for Athabasca Valles, Mars

Details Testing the Late-Stage Outflow Channel Origin Hypothesis: Investigating Both Water Erosion and Lava Erosion Origins for Athabasca Valles, Mars Testing the Late-Stage Outflow Channel Origin Hypothesis: Investigating Both Water Erosion and Lava Erosion Origins for Athabasca Valles, Mars

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1056h&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1056

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Analytical models estimate the fluid volumes, effusion rates, and
erosion rates required to erode Athabasca Valles by water and by lava.
Results are put in context with geomorphologic observations to assess
the potential for each origin hypothesis.

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