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• W1817868867 abstract "Summary: The utility of Kr and Xe measurement are severalfold: (i) We hope to improve upon the at-mospheric measurements from Viking (and refine-ments of those measurements using martian meteor-ites); (ii) We hope to measure minor isotope abun-dances to determine the influence on the atmosphere of impact vaporization of spallogenic Kr and Xe isotopes; (iv) If spallogenic contributions to the atmosphere are small, then mass fractionation of Xe could be more precisely determined; and (v) A better mass fractiona-tion determination will result in a better estimation of the fission Xe component in the martian atmosphere. SAM provides an opportunity to measure both atmos-pheric Kr and Xe and that thermally evolved from solid n-tamination. The static operation, chemical scrubbing and gettering will facilitate the separation and then trapping of Kr and Xe for analysis on Mars with the potential to in-form our continued quest for understanding of the accre-tionary and evolutionary processes that affect the devel-opment of habitable planets." @default.
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• W1817868867 date "2013-03-18" @default.
• W1817868867 modified "2023-10-03" @default.
• W1817868867 title "Heavy noble gas measurements on Mars with SAM" @default.
• W1817868867 hasPublicationYear "2013" @default.
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