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Genesis of howardites, diogenites, and eucritesThe reported investigation was mainly concerned with the precise determinations of major-, minor-, and trace-element abundances, especially the REE abundances in the bulk howardites in order to establish the bulk rock composition for the future chemical-mineralogical, petrographic studies of different rock types on the chemically unique howardites and diogenites if they exist. From the chemical data for the major-element abundances and the REE patterns of the howardites analyzed, it is evident that these howardites are predominantly composed of eucritic and diogenitic components. The analytical results for howardites and diogenites are shown in two tables together with the results for CRB-1. The chondritic normalized K, Sr, Ba, REE, Hf, and Sc abundances of these howardites are plotted in two graphs.
Document ID
19780057656
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Fukuoka, T.
(Oregon State Univ. Corvallis, OR, United States)
Boynton, W. V.
(Oregon State Univ. Corvallis, OR, United States)
Ma, M.-S.
(Oregon State Univ. Corvallis, OR, United States)
Schmitt, R. A.
(Oregon State University Corvallis, Ore., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1977
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 14, 1977
End Date: March 18, 1977
Accession Number
78A41565
Funding Number(s)
CONTRACT_GRANT: NGL-38-002-039
CONTRACT_GRANT: NGL-38-002-020
Distribution Limits
Public
Copyright
Other

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