Oxygen Isotopic Evolution in the Early Solar Nebula: Validation of the H2O Transport Model

Details Oxygen Isotopic Evolution in the Early Solar Nebula: Validation of the H2O Transport Model Oxygen Isotopic Evolution in the Early Solar Nebula: Validation of the H2O Transport Model

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1016..409f&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From

Computer Science

Interstellar Medium And Nebulae In External Galaxies, Numerical Approximation And Analysis, Meteors, Meteorites And Tektites

Scientific paper

We perform a numerical simulation on the global transport process of
16O-poor H2O and silicate in a protoplanetary disk
to examine whether the process is responsible for the oxygen isotopic
systematics observed in chondritic components without conflicting with
observation of protoplanetary disks and theory of planet formation.

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