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Apollo 14 - Some geochemical aspects.Chemical analyses have been obtained for five samples of Apollo 14 regolith fines, three 14230 core samples, 14049 soil clod, 14305 and 14319 breccias, 14310 basalt, and some separated phases. The chemical uniformity of these Apollo 14 samples indicates thorough mixing and/or uniform source rocks. Basalt 14310 can be matched well in composition by a four-to-one mixture of soil and plagioclase. Eu(2+)/Eu(3+) ratios calculated for 14310 pigeonite and plagioclase are similar to those for Apollo 12 and 15 mare-type basalt phases; this indicates similar redox conditions. The investigated Apollo 14 samples are chemically similar to Apollo 12 and 15 KREEP as distinct from Apollo 11, 12, and 15, and Luna 16 mare-type basalts. A relationship between the two types of basalt, in which mare-basalts would represent fused cumulates, is suggested.
Document ID
19730034959
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Philpotts, J. A.
Schnetzler, C. C.
Nava, D. F.
Bottino, M. L.
Fullagar, P. D.
Thomas, H. H.
Schuhmann, S.
Kouns, C. W.
(NASA Goddard Space Flight Center Planetology Branch, Greenbelt, Md., 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
73A19761
Distribution Limits
Public
Copyright
Other

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