Eruption Constraints for a Young Channelized Lava Flow, Marte Vallis, Mars

Details Eruption Constraints for a Young Channelized Lava Flow, Marte Vallis, Mars Eruption Constraints for a Young Channelized Lava Flow, Marte Vallis, Mars

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1112t&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1112

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Scientific paper

This 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.

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