The Oxygen Isotope Evolution of Our Galaxy: Implications for the Interpretation of Early Solar System Heterogeneities

Details The Oxygen Isotope Evolution of Our Galaxy: Implications for the Interpretation of Early Solar System Heterogeneities The Oxygen Isotope Evolution of Our Galaxy: Implications for the Interpretation of Early Solar System Heterogeneities

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1804j&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

1

Scientific paper

The observed range of oxygen isotopes in early solar system materials
can be explained with a simple galactic evolution model for oxygen
isotopes. What is required is a mean residence time of the oxygen in the
dust of the interstellar medium of about 0.5

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