Groundwater Depth, Cryosphere Thickness, and Crustal Heat Flux in the Epoch of Ravi Vallis, Mars

Details Groundwater Depth, Cryosphere Thickness, and Crustal Heat Flux in the Epoch of Ravi Vallis, Mars Groundwater Depth, Cryosphere Thickness, and Crustal Heat Flux in the Epoch of Ravi Vallis, Mars

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2163c&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2163

Physics

1

Scientific paper

We propose a method to estimate the cryosphere and groundwater depth via
analysis of chaotes that formed in outflow channels. We derive a range
of 700 to 1000 m for Iamuna Chaos in Ravi Vallis, and estimate the local
Hesperian crustal heat flux was 30 to 50 mW m2.

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