Low Pressure Adsorption of Ar, Kr and Xe on Kerogen: Implications for the Trapping of Noble Gases onto Meteoritic Matter

Details Low Pressure Adsorption of Ar, Kr and Xe on Kerogen: Implications for the Trapping of Noble Gases onto Meteoritic Matter Low Pressure Adsorption of Ar, Kr and Xe on Kerogen: Implications for the Trapping of Noble Gases onto Meteoritic Matter

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1699m&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1699

Physics

Scientific paper

Low pressure adsorption (i.e. solar nebula) of Ar, Kr and Xe on kerogen
(Q analog) suggest that for environmental temperatures < 80K ,
adsorption could well be responsible for the concentration and
subsequent trapping of noble gases in Q.

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