Cometary Refractories, Crystalline Silicates, Short-lived Radioactivities, Stable Oxygen Isotopes, and the Solar Nebula

Details Cometary Refractories, Crystalline Silicates, Short-lived Radioactivities, Stable Oxygen Isotopes, and the Solar Nebula Cometary Refractories, Crystalline Silicates, Short-lived Radioactivities, Stable Oxygen Isotopes, and the Solar Nebula

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1021b&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

Mixing in a marginally gravitationally unstable disk can explain
refractories in comets, crystalline silicates in outer disks,
homogeneity of short-lived radioisotopes, and stable oxygen isotope
anomalies.

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