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Composition and origin of Luna 16 aluminous mare basaltsThe mineralogy and petrology of 58 lithic fragments, 52 of which are basaltic, in the Luna 16 samples were studied, with textures, and mineral and bulk compositions determined by petrographic and electron microprobe techniques. These mare basalt fragments differ from other mare basalts in being aluminous (11-20%) which results in plagioclase and (olivine) microphenocrysts; moreover, they have very low-FeO and MgO and high-CaO, FeO/MgO, and normative diopside contents.
Document ID
19770051877
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Kurat, G.
(New Mexico Univ. Albuquerque, NM, United States)
Kracher, A.
(Naturhistorisches Museum Vienna, Austria)
Keil, K.
(New Mexico Univ. Albuquerque, NM, United States)
Warner, R.
(New Mexico, University Albuquerque, N. Mex., United States)
Prinz, M.
(American Museum of Natural History New York, N.Y., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1976
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 15, 1976
End Date: March 19, 1976
Accession Number
77A34729
Funding Number(s)
PROJECT: OFFWF PROJECT 2272
OTHER: NGL-32-004-063
Distribution Limits
Public
Copyright
Other

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