Tying Up Loose Ends in Chondrule Formation by Shocks

Details Tying Up Loose Ends in Chondrule Formation by Shocks Tying Up Loose Ends in Chondrule Formation by Shocks

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2300m&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

We discuss two unresolved issues in modeling nebular shocks: the
appropriate input radiation boundary condition and the dust opacity.
Resolving these issues and line cooling now allows a full calculation of
shock-heated chondrule thermal histories.

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