Abiotic Origin for PAHs and Aliphatic Hydrocarbons in ALH84001 and Nakhla Martian Meteorites: Synthesis in Trapped Magmatic and/or Impact Gases

Details Abiotic Origin for PAHs and Aliphatic Hydrocarbons in ALH84001 and Nakhla Martian Meteorites: Synthesis in Trapped Magmatic and/or Impact Gases Abiotic Origin for PAHs and Aliphatic Hydrocarbons in ALH84001 and Nakhla Martian Meteorites: Synthesis in Trapped Magmatic and/or Impact Gases

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1879z&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1879

Physics

Scientific paper

We argue that hydrocarbons in ALH84001 could have formed metastably from
CO (CO 2) and H2 in cooling magmatic and/or impact gases. The origin of
hydrocarbons in Nakhla is unclear, but the trapped-gases hypothesis
seems to be possible.

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