Krypton and Xenon in Martian Meteorites from Hot Deserts -- The Low Temperature Component

Details Krypton and Xenon in Martian Meteorites from Hot Deserts -- The Low Temperature Component Krypton and Xenon in Martian Meteorites from Hot Deserts -- The Low Temperature Component

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1532m&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1532

Computer Science

3

Scientific paper

Low temperature Kr and Xe signatures of martian meteorites from hot
deserts are commonly explained by a mixture of Chassigny and Air type
gases. But an elementally fractionated Air component (EFA) like that in
ALH 84001 and Nakhlites but of terrestrial origin, can also explain
these signatures.

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