Oxygen isotopic anomaly and solar nebular photochemistry

Details Oxygen isotopic anomaly and solar nebular photochemistry Oxygen isotopic anomaly and solar nebular photochemistry

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983m%26p....29..199k&link_type=abstract

Moon and the Planets (ISSN 0165-0807), vol. 29, Oct. 1983, p. 199-202.

Physics

7

Isotope Effect, Oxygen Isotopes, Photochemical Reactions, Reaction Kinetics, Solar Corona, Anomalies, Carbonaceous Meteorites, Meteoritic Composition, Shock Wave Interaction, Solar Physics

Scientific paper

At the cool periphery of the solar nebula, oxygen could be formed photochemically from water. The mixing of 17O and 18O enriched by the self-shielding effect of 16O2 to the dust grain melted by the shock waves there would explain the oxygen isotopic anomaly in the high-temperature mineral of the carbonaceous meteorites.

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