Shock Chemistry in the Inner Solar Nebula: Implications for Meteorites and Protoplanetary Disks

Details Shock Chemistry in the Inner Solar Nebula: Implications for Meteorites and Protoplanetary Disks Shock Chemistry in the Inner Solar Nebula: Implications for Meteorites and Protoplanetary Disks

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.2096k&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.2096

Physics

Scientific paper

We calculate the gas-phase chemical abundances behind chondrule-forming
(7-8 km/sec) shocks. We discuss the consequences on the chemistry of the
terrestrial-planet-forming regions of protoplanetary disks.

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