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Composition and origin of Nuevo Laredo Trend eucritesThe new bulk-rock analyses reported for the ALHA81001, Lakangaon and Nuevo Laredo eucritic meteorites indicate that the first of these resembles Ibitira in possessing lower Na concentrations than any other eucrite, while the other two are the lowest-Mg/Fe of all eucrites. The present data and those seen in the literature suggest that most of the ostensible Main Group eucrites actually belong to the Nuevo Laredo Trend, which is characterized by limited variations of incompatible element contents despite considerable variations in Mg/(Mg+Fe) ratio and V content.
Document ID
19870052296
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0016-7037(87)90082-2
Authors
Warren, Paul H. (California Univ. Los Angeles, CA, United States)
Jerde, Eric A. (California, University Los Angeles, United States)
Date Acquired
August 13, 2013
Publication Date
March 1, 1987
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 51
ISSN: 0016-7037
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0016-7037
Accession Number
87A39570
Funding Number(s)
CONTRACT_GRANT: NAG9-87
CONTRACT_GRANT: NAG9-96
Distribution Limits
Public
Copyright
Other

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