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The CR (Renazzo-type) carbonaceous chondrite group and its implicationsA petrologic, geochemical, and oxygen isotropic study of the CR chondrites including Renazzo, Al Rais, El Djouf 001 and the paired Acfer meteorites, EET87770 and the paired samples, MAC87320, Y790112, Y793495, and Y791498 is presented. It is concluded that the CR group is characterized by abundant large multilayered, Fe, Ni metal-rich, type I chondrules; abundant matrix and dark inclusions; unique assemblages of serpentine and chlorite-rich phyllosilicates and Ca-carbonates; Ca-carbonate rims on chondrules; abundant Fe, Ni metal with a positive Ni vs. Co trend and a solar Ni:Co ratio; and amoeboid olivine aggregates with Mn-rich and Mn-poor forsterite.
Document ID
19930052989
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Weisberg, Michael K.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Prinz, Martin
(American Museum of Natural History New York, United States)
Clayton, Robert N.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Mayeda, Toshiko K.
(Chicago Univ. IL, United States)
Date Acquired
August 16, 2013
Publication Date
April 1, 1993
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 57
Issue: 7
ISSN: 0016-7037
Subject Category
Lunar And Planetary Exploration
Accession Number
93A36986
Funding Number(s)
CONTRACT_GRANT: NAG9-32
CONTRACT_GRANT: NSF EAR-89-20584
Distribution Limits
Public
Copyright
Other

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