Stardust in Fine-Grained Chondrule Rims and Matrix in LaPaz 031117: Insights Into the Conditions of Dust Accretion in the Solar Nebula

Details Stardust in Fine-Grained Chondrule Rims and Matrix in LaPaz 031117: Insights Into the Conditions of Dust Accretion in the Solar Nebula Stardust in Fine-Grained Chondrule Rims and Matrix in LaPaz 031117: Insights Into the Conditions of Dust Accretion in the Solar Nebula

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1107h&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1107

Physics

Scientific paper

Abundances of presolar SiC and oxides are similar in the matrix and a
chondrule rim of LAP 031117, but presolar silicate abundances are higher
in the matrix. Silicates may have been destroyed during accretion of the
rim onto a still hot chondrule.

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