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Mare basalts from the Taurus-Littrow region of the moonTwo distinct chemical basalt types have been sampled at the Apollo 17 landing site. Very high-titanium basalts (about 13 wt % TiO2) are the dominant type and display a textural range from olivine-porphyritic, ilmenite vitrophyres to plagioclase-poikilitic, ilmenite microgabbros. Most of these rocks could have come from one flow. These basalts appear to represent partial melts from feldspar-ilmenite cumulates with an Ar-40/Ar-39 age of about 3.7 G.y., which have experienced little, if any, near-surface fractionation of olivine and Fe-Mg-Ti oxides. A second type of basalt virtually identical to the Apollo 11 (low-K) basalts is much less common.
Document ID
19750055499
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Papike, J. J.
Bence, A. E.
Lindsley, D. H.
(New York, State University Stony Brook, N.Y., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1974
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 18, 1974
End Date: March 22, 1974
Accession Number
75A39571
Funding Number(s)
CONTRACT_GRANT: NGL-33-015-130
Distribution Limits
Public
Copyright
Other

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