Oxidizing Proto-Titan: Constraint from the Impact Origin of Its N2 Atmosphere

Details Oxidizing Proto-Titan: Constraint from the Impact Origin of Its N2 Atmosphere Oxidizing Proto-Titan: Constraint from the Impact Origin of Its N2 Atmosphere

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1358i&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1358

Computer Science

Scientific paper

We show that a CO2-rich oxidizing proto-atmosphere is necessary to form
Titan’s current N2 atmosphere by impact shock heating, implying
that the chemical composition of satellitesimals that formed the
saturnian system containing Titan should be oxidizing.

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