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Sample 67955 - A description and a problemClasts in breccia sample 67955 contain relatively coarse olivine and plagioclase in part enveloped by poikilitic hypersthene and diopside. This distinctive texture is concluded to result from high temperature crystallization in the presence of a fluid phase, probably a silicate melt. A problem posed by this rock is whether the bulk chemistry, characterized by a high Mg/Fe ratio but low total Fe + Mg, is the result of primary igneous processes on the moon or whether it is the residual end product of a multiple distillation process resulting from repeated meteorite impacts.
Document ID
19740040098
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Hollister, L. S.
(Princeton University Princeton, N.J., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Subject Category
Space Sciences
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 5, 1973
End Date: March 8, 1973
Accession Number
74A22848
Funding Number(s)
CONTRACT_GRANT: NGR-31-001-205
Distribution Limits
Public
Copyright
Other

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