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Isotope analysis of crystalline impact melt rocks from Apollo 16 stations 11 and 13, North Ray CraterThe North Ray Crater Target Rock Consortium was formed to study a large number of rake samples collected at Apollo 16 stations 11 and 13 with comparative chemical, mineralogical, and chronological techniques in order to provide a larger data base for the discussion of lunar highland evolution in the vicinity of the Apollo 16 landing region. The present investigation is concerned with Rb-Sr and Sm-Nd isotopic analyses of a number of whole-rock samples of feldspathic microporhyritic (FM) impact melt, a sample type especially abundant among the North Ray crater (station 11) sample collection. Aspects of sample mineralogy and analytical procedures are discussed, taking into account FM impact melt rocks 6715 and 63538, intergranular impact melt rock 67775, subophitic impact melt rock 67747, subophitic impact melt rock 67559, and studies based on the utilization of electron microscopy and mass spectroscopy.
Document ID
19850047882
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Reimold, W. U.
(Witwatersrand, University Johannesburg, Republic of South Africa; Muenster, University, Muenster, Germany)
Nyquist, L. E.
(NASA Johnson Space Center Houston, TX, United States)
Bansal, B. M.
(Witwatersrand Univ. Johannesburg, South Africa)
Shih, C.-Y.
(Witwatersrand Univ. Johannesburg, South Africa)
Weismann, H.
(Lockheed Electronics Corp. Houston, TX, United States)
Wooden, J. L.
(U.S. Geological Survey, Menlo Park, CA; Lockheed Electronics Corp. Houston, TX, United States)
Mackinnon, I. D. R.
(Microbeam, Inc. Houston, TX, United States)
Date Acquired
August 12, 2013
Publication Date
February 15, 1985
Publication Information
Publication: Journal of Geophysical Research, Supplement
Volume: 90
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
85A30033
Distribution Limits
Public
Copyright
Other

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