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Electron petrography of Apollo 14 and 15 rocks.Comparative optical and high-voltage electron petrographic analyses of igneous rocks and several types of breccias the Fra Mauro and Apennine sites of Apollo 14 and 15 are reported and interpreted. The crystalline rocks are found to differ substantially from the Apollo 11 and 12 basalts. Substructures in the Apollo 14 breccias are complex. At least two bonding mechanisms can be discerned from the electron petrographic examination: (a) 'shock sintering' due to high pressures and temperatures associated with the shock waves of meteoritic impacts; and (b) lithification by glass bonding.
Document ID
19730034900
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Lally, J. S.
Fisher, R. M.
(United States Steel Research Laboratories Monroeville, Pa., United States)
Christie, J. M.
Griggs, D. T.
(California, University Los Angeles, Calif., United States)
Heuer, A. H.
Nord, G. L., Jr.
Radcliffe, S. V.
(Case-Western-Reserve University Cleveland, Ohio, 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
73A19702
Distribution Limits
Public
Copyright
Other

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