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Isotopic and chemical investigations on Angra dos ReisIsotope ratios and chemical abundance measurements for a variety of elements are reported for total meteorite and mineral separates of the Angra dos Reis achondrite. U-Pb, Th-Pb, and Pb-Pb ages are concordant at 4.54 eons for the total meteorite and for high-purity whitlockite, which indicates that Angra dos Reis is an early planetary differentiate that has not been disturbed for these systems since 4.54 eons ago. The implications of different ratios of Sr-87 and Sr-86 found in different components are discussed. Xe isotopic measurements show that Pu-244 was enriched in the whitlockite relative to the pyroxene by a factor of about 18. Chemical enrichment factors between the whitlockite and the fassaitic pyroxene in Angra dos Reis are presented
Document ID
19770056177
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wasserburg, G. J.
(California Inst. of Tech. Pasadena, CA, United States)
Tera, F.
(California Inst. of Tech. Pasadena, CA, United States)
Papanastassiou, D. A.
(California Inst. of Tech. Pasadena, CA, United States)
Huneke, J. C.
(California Institute of Technology Pasadena, Calif., United States)
Date Acquired
August 9, 2013
Publication Date
June 1, 1977
Publication Information
Publication: Earth and Planetary Science Letters
Volume: 35
Issue: 2, Ju
Subject Category
Lunar And Planetary Exploration
Accession Number
77A39029
Funding Number(s)
CONTRACT_GRANT: NSF PHY-76-02724
CONTRACT_GRANT: NGL-05-002-188
Distribution Limits
Public
Copyright
Other

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