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The origin of metal clasts in the Bencubbin meteoritic brecciaThe Bencubbin meteorite is a shock-welded breccia consisting of a diverse collection of metal and silicate clasts. Several types of evidence suggest that the metal clasts in Bencubbin retain chemical abundances that were established during condensation. The Cr, Ni, P and trace element abundances are consistent with condensation calculations and are much closer to the predicted compositions of metal condensates than the CM metal particles. In addition, petrographic and chemical evidence strongly suggest that the breccia components were incorporated as solid clasts within the breccia prior to a shock heating event of very short duration, which did not produce significant metamorphic effects.
Document ID
19790054074
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Newsom, H. E.
(Arizona Univ. Tucson, AZ, United States)
Drake, M. J.
(Arizona, University Tucson, Ariz., United States)
Date Acquired
August 9, 2013
Publication Date
May 1, 1979
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 43
Subject Category
Lunar And Planetary Exploration
Accession Number
79A38087
Funding Number(s)
CONTRACT_GRANT: NGL-03-002-388
Distribution Limits
Public
Copyright
Other

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