The Trapping of Ar, Kr, and Xe in Martian Clathrates and the Possibility of Detecting Clathrates on Mars by Seasonal Changes in the Xe/Kr Ratio

Details The Trapping of Ar, Kr, and Xe in Martian Clathrates and the Possibility of Detecting Clathrates on Mars by Seasonal Changes in the Xe/Kr Ratio The Trapping of Ar, Kr, and Xe in Martian Clathrates and the Possibility of Detecting Clathrates on Mars by Seasonal Changes in the Xe/Kr Ratio

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1660s&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

1

Scientific paper

Calculations show that Xe would be much more readily trapped in multiple
guest clathrates on Mars than would be Kr. Measurement of the Xe/Kr
ratio over the course of a martian year would be a sensitive detector of
seasonal formation of clathrate.

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