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Apollo 17 high-Ti mare basalts - New bulk compositional data, magma types, and petrogenesisBulk compositional and mineral chemical data for 28 previously unanalyzed samples support the classification of Apollo-17 high-Ti mare basalts into three-types (A, B, and C), defined on the basis of analyses of fine-grained basalts. The most MgO- and TiO2-rich fine-grained basalts of these types appear to be the best choices for representing the compositions of the parent magmas.
Document ID
19800039395
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Warner, R. D. (New Mexico Univ. Albuquerque, NM, United States)
Taylor, G. J. (New Mexico Univ. Albuquerque, NM, United States)
Conrad, G. H. (New Mexico Univ. Albuquerque, NM, United States)
Northrop, H. R. (New Mexico Univ. Albuquerque, NM, United States)
Barker, S. (New Mexico Univ. Albuquerque, NM, United States)
Keil, K. (New Mexico, University Albuquerque, N. Mex., United States)
Ma, M.-S. (New Mexico Univ. Albuquerque, NM, United States)
Schmitt, R. (Oregon State University Corvallis, Ore., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1979
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 19, 1979
End Date: March 23, 1979
Accession Number
80A23565
Funding Number(s)
CONTRACT_GRANT: NGL-32-002-039
CONTRACT_GRANT: NGL-32-004-063
Distribution Limits
Public
Copyright
Other

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