Hydrogen Isotopic Exchange Rates Between Deuterium-rich Sources (UV Irradiated Molecular Hydrogen and Liquid Water) and an Organic Molecule: Implications for the Conditions of Formation of the Insoluble Organic Matter in the Early Solar System

Details Hydrogen Isotopic Exchange Rates Between Deuterium-rich Sources (UV Irradiated Molecular Hydrogen and Liquid Water) and an Organic Molecule: Implications for the Conditions of Formation of the Insoluble Organic Matter in the Early Solar System Hydrogen Isotopic Exchange Rates Between Deuterium-rich Sources (UV Irradiated Molecular Hydrogen and Liquid Water) and an Organic Molecule: Implications for the Conditions of Formation of the Insoluble Organic Matter in the Early Solar System

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2001t&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

1

Scientific paper

The rate of deuterium exchange between the C-H bonds of the insoluble
organic matter (IOM) and H3+ confirm the
interpretation according to which IOM could get its deuterium in the
dense and UV irradiated protosolar disk.

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