The Oxygen Isotopic Composition of the Sun and Implications for Oxygen Processing in Molecular Clouds, Star-forming Regions, and the Solar Nebula

Details The Oxygen Isotopic Composition of the Sun and Implications for Oxygen Processing in Molecular Clouds, Star-forming Regions, and the Solar Nebula The Oxygen Isotopic Composition of the Sun and Implications for Oxygen Processing in Molecular Clouds, Star-forming Regions, and the Solar Nebula

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1572i&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1572

Computer Science

Scientific paper

The solar oxygen isotopic composition is depleted in 16O by 54 permil
relative to terrestrial. This composition can be explained by molecular
cloud predissociation and gas-solid fractionation during formation of
the accretion disk.

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