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Pyroxenes from breccia 14303.Review of the investigation results obtained on the adjacent polished thin sections 47 and 53 of breccia 14303, the largest rock returned by Apollo 14 for which a location has not been established. A basaltic lithic clast, composed mainly of plagioclase, olivine, and pigeonite zoned to subcalcic augite, is found to occupy the same relative position in both sections and is assumed to represent a single lithic chip. Further study of lithic and fragmental clasts in breccias is seen likely to yield information on lunar history between 4.6 and 3.9 b.y. ago.
Document ID
19730034903
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Weigand, P. W.
Hollister, L. S.
(Princeton University Princeton, N.J., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1972
Subject Category
Space Sciences
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: January 10, 1972
End Date: January 13, 1972
Accession Number
73A19705
Funding Number(s)
CONTRACT_GRANT: NGR-31-001-205
Distribution Limits
Public
Copyright
Other

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