Particle Formation and 16O Enrichment from the Inner Rim of the Solar Nebula

Details Particle Formation and 16O Enrichment from the Inner Rim of the Solar Nebula Particle Formation and 16O Enrichment from the Inner Rim of the Solar Nebula

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1135l&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1135

Physics

Scientific paper

The Jet Flow Model is used to deduce an evolutionary track on the oxygen
three-isotope diagram. In terms of age, the model predicts that ordinary
chondrite chondrules > enstatite chondrules > carbonaceous
chondrite chondrules.

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