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Oxygen isotopic heterogeneities, their petrological correlations, and implications for melt origins of chondrules in unequilibrated ordinary chondritesClayton et al. (1976, 1982) established that equilibrated ordinary chondrites (EOC's) can be divided into the H- and L-groups on the basis of their oxygen isotopic composition. The present investigation is concerned with new oxygen isotopic analyses of petrologically well-characterized individual chondrules from the unequilibrated chondrites Dhajala (H3,4), Hallingeberg (L3), and Semarkona (LL3). A study is conducted regarding the implications of isotopic/petrologial correlations for the origin of chondrules in ordinary chondrites. It is found that the oxygen isotopic heterogeneities among chondrules are reminiscent of the bulk elemental and phase compositional heterogeneities among the same and other chondrules as reported by Gooding et al. (1979, 1980). It is concluded that chondrules formed possibly as a result of the melting of preexisting materials which were both chemically and isotopically heterogeneous.
Document ID
19840033957
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Gooding, J. L.
(NASA Johnson Space Center Planetary Materials Branch, Houston, TX, United States)
Mayeda, T. K.
(Chicago Univ. Chicago, IL, United States)
Clayton, R. N.
(Chicago, University Chicago, IL, United States)
Fukuoka, T.
(Gakushuin University Tokyo, Japan)
Date Acquired
August 12, 2013
Publication Date
November 1, 1983
Publication Information
Publication: Earth and Planetary Science Letters
Volume: 65
Issue: 2
ISSN: 0012-821X
Subject Category
Lunar And Planetary Exploration
Accession Number
84A16744
Funding Number(s)
CONTRACT_GRANT: NSF EAR-78-23680
CONTRACT_GRANT: NGL-32-002-039
CONTRACT_GRANT: NGL-32-004-064
Distribution Limits
Public
Copyright
Other

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