The Stardust Inventories of CR Chondrites QUE 99177 and MET 00426, and the Distribution of Presolar Silicate and Oxide Grains in the Early Solar System

Details The Stardust Inventories of CR Chondrites QUE 99177 and MET 00426, and the Distribution of Presolar Silicate and Oxide Grains in the Early Solar System The Stardust Inventories of CR Chondrites QUE 99177 and MET 00426, and the Distribution of Presolar Silicate and Oxide Grains in the Early Solar System

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1280f&link_type=abstract

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

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Scientific paper

Stardust abundances in QUE 99177 and MET 00426 are high, consistent with
their low degrees of aqueous alteration. Both also have presolar
silicate/oxide ratios that are significantly higher than those
previously found in other primitive meteorites.

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