Contents of Highly Labile Trace Elements in H4-6 Chondrite Falls Are Not Affected by Post-Accretionary Heating

Details Contents of Highly Labile Trace Elements in H4-6 Chondrite Falls Are Not Affected by Post-Accretionary Heating Contents of Highly Labile Trace Elements in H4-6 Chondrite Falls Are Not Affected by Post-Accretionary Heating

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1110w&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1110

Physics

Scientific paper

Contents of volatile trace elements in H4-6 chondrites were established
during nebular condensation and accretion and the most thermally labile
of these were unaffected by metamorphism of their parent bodies, shock
heating or close solar approach.

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