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Oxygen isotope relationships in iron meteoritesIron meteorites with oxygen-bearing phases can be classified in terms of their oxygen isotopic abundances. These iron meteorite classes are isotopically similar to various stony meteorite classes, which may indicate a common origin. The group IAB and IIICD irons may be related to the winonaites; group IIE irons may be related to H chondrites; group IVA irons may be related to L or LL chondrites.
Document ID
19840033959
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0012-821X(83)90161-9
Authors
Clayton, R. N. (Chicago Univ. Chicago, IL, United States)
Mayeda, T. K. (Chicago, University Chicago, IL, United States)
Olsen, E. J. (Field Museum of Natural History Chicago, IL, United States)
Prinz, M. (American Museum of Natural History New York, NY, United States)
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
84A16746
Funding Number(s)
CONTRACT_GRANT: NAG9-32
CONTRACT_GRANT: NSF EAR-78-23680
Distribution Limits
Public
Copyright
Other

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