A Heterogeneous Chemical Origin for 16O Enriched and 16O Depleted Reservoirs in the Early Solar System

Details A Heterogeneous Chemical Origin for 16O Enriched and 16O Depleted Reservoirs in the Early Solar System A Heterogeneous Chemical Origin for 16O Enriched and 16O Depleted Reservoirs in the Early Solar System

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1992d&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1992

Physics

Scientific paper

I propose that the 16O-rich and 16O-poor reservoirs present in the early
solar system were produced by heterogeneous chemical reactions that
produce H2O on the surface of interstellar dust grains in dense
molecular clouds.

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