Adiabatic Shock Waves in Icy Regions of the Solar Nebula: Implications for Origins of Phyllosilicate Minerals in Primitive Meteorites

Details Adiabatic Shock Waves in Icy Regions of the Solar Nebula: Implications for Origins of Phyllosilicate Minerals in Primitive Meteorites Adiabatic Shock Waves in Icy Regions of the Solar Nebula: Implications for Origins of Phyllosilicate Minerals in Primitive Meteorites

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1243c&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1243

Physics

Scientific paper

We re-examine the possibility that phyllosilicate minerals, such as
those found in the chondrule rims in CM chondrites, formed in the solar
nebula. Specifically, we consider the formation in the presence of water
vapor produced by a shock wave that could have also formed chondrules.

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