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Very low-Ti mare basaltsBulk compositions, petrology, and mineralogy of lithic fragments discovered in polished sections of Apollo 17 drill core samples 70007, 70008, and 70009 and Luna 24 soil 24077, 43 are described. The fragments have unambiguous affinities to mare basalts, but are exceptionally low in TiO2 (less than 1.0 wt.% TiO2). Apollo 17 rake sample 78526 is a green glassy rock of similar composition. Together the samples represent a distinct variety of mare basalts. Bulk compositional relationships suggest that they are related to Apollo 15 green glass, but the data do not permit one to discern the precise nature of the relationship. Both fractional crystallization and partial melting models can explain the observed compositional trends.
Document ID
19770054949
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Taylor, G. J.
(New Mexico Univ. Albuquerque, NM, United States)
Keil, K.
(New Mexico Univ. Albuquerque, NM, United States)
Warner, R. D.
(New Mexico, University Albuquerque, N. Mex., United States)
Date Acquired
August 9, 2013
Publication Date
June 1, 1977
Publication Information
Publication: Geophysical Research Letters
Volume: 4
Subject Category
Lunar And Planetary Exploration
Accession Number
77A37801
Funding Number(s)
CONTRACT_GRANT: NGL-32-004-063
Distribution Limits
Public
Copyright
Other

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