Heat-Treatment of MgSiO Smokes of Astrophysical Interest: Possible Implications for Olivine-Pyroxene-Silica Assemblages in Chondritic Aggregate IDPs

Details Heat-Treatment of MgSiO Smokes of Astrophysical Interest: Possible Implications for Olivine-Pyroxene-Silica Assemblages in Chondritic Aggregate IDPs Heat-Treatment of MgSiO Smokes of Astrophysical Interest: Possible Implications for Olivine-Pyroxene-Silica Assemblages in Chondritic Aggregate IDPs

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1322r&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1322

Astronomy and Astrophysics

Astrophysics

Scientific paper

Anhydrous silicates in coarse-grained ferromagnesiosilica PCs formed
during atmospheric entry flash-heating also constrain the
astromineralogy of astrophysical dust. This is because of the unique
closed-system behavior of these PCs in chondrtitic aggregate IDPs.

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