Sensitivity of D/H in Mars Atmosphere to Time Varying Processes in the Water Cycle, Water Reservoir Sizes and Exchange Rates; What D/H History Might be Found by Drilling in the North Polar Cap and What It Might Mean

Details Sensitivity of D/H in Mars Atmosphere to Time Varying Processes in the Water Cycle, Water Reservoir Sizes and Exchange Rates; What D/H History Might be Found by Drilling in the North Polar Cap and What It Might Mean Sensitivity of D/H in Mars Atmosphere to Time Varying Processes in the Water Cycle, Water Reservoir Sizes and Exchange Rates; What D/H History Might be Found by Drilling in the North Polar Cap and What It Might Mean

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpico1323.8004f&link_type=abstract

Fourth International Conference on Mars Polar Science and Exploration, October 2-6, 2006, Davos, Switzerland. LPI Contribution

Physics

Scientific paper

A time varying stable isotope model for the D/H history of Mars water
cycle is developed with variable atmosphere, space loss rate, ground
and ice cap flux rates. It considers coupled ground reservoirs and
traces D/H in the air and reservoirs secularly and over obliquity
cycles.

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