Will Organic Synthesis Within Icy Grains or on Dust Surfaces Within the Primitive Solar Nebula Completely Erase the Effects of Photochemical Self Shielding?

Details Will Organic Synthesis Within Icy Grains or on Dust Surfaces Within the Primitive Solar Nebula Completely Erase the Effects of Photochemical Self Shielding? Will Organic Synthesis Within Icy Grains or on Dust Surfaces Within the Primitive Solar Nebula Completely Erase the Effects of Photochemical Self Shielding?

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1495n&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1495

Physics

Scientific paper

Self shielding relies on the differential dissociation of CO and
sequestration of ^1^6O-rich CO. Organic synthesis in the solar nebula
starts with CO and hydrogen on grain surfaces, producing hydrocarbons
and water. ^1^6O-rich CO cannot be sequestered.

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