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Comparative petrology and possible genetic relations among the Apollo 11 basaltsA comparative petrological study has been performed on 19 large Apollo-11 basalt fragments as well as two smaller vitrophyres in order to determine how many igneous bodies are presented by this suite of rocks. Detailed petrographic and mineral chemical studies have been performed on each sample along with an electron microprobe point count, which gives the mode, the range and distribution of all mineral zonation and the bulk composition. These data confirm the twofold division of the Apollo-11 basalts into high-K (type A) and low-K (type B) basalts.
Document ID
19790055111
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Beaty, D. W.
(California Inst. of Tech. Pasadena, CA, United States)
Albee, A. L.
(California Institute of Technology Pasadena, Calif., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1978
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 13, 1978
End Date: March 17, 1978
Accession Number
79A39124
Funding Number(s)
CONTRACT_GRANT: NGL-05-002-338
Distribution Limits
Public
Copyright
Other

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