Thermal Processing and Accretion of Silicate Dust into Chondrites and Comets

Details Thermal Processing and Accretion of Silicate Dust into Chondrites and Comets Thermal Processing and Accretion of Silicate Dust into Chondrites and Comets

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2007s&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2007

Physics

1

Scientific paper

Matrices of primitive chondrites resemble crystalline and amorphous
silicates in IDPs and probably condensed in chondrule-forming regions.
This favors shock formation at 2-3 AU and rim accretion after matrix
silicates were mixed with sticky organics.

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