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Ion microprobe studies of trace elements in Apollo 14 volcanic glass beads - Comparisons to Apollo 14 mare basalts and petrogenesis of picritic magmasResults are presented from trace element analysis, by ion microprobe techniques, of individual glass beads representing seven compositionally distinct types of picritic glass beads from the Apollo 14 landing site. The picritic glass beads at the A-14 exhibited a wide range of primary magma compositions and a lack of petrogenetic linkage (via crystal fractionation) to crystalline basalts. The wide range of major and trace element characteristics of the picritic glass beads is consistent with derivation from mineralogically distinct sources which consist of varying proportions of olivine + orthopyroxene +/- clonopyroxene +/- ilmenite +/- plagioclase +/- KREEP component.
Document ID
19900043794
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Shearer, C. K.
(South Dakota School of Mines and Technology Rapid City, SD, United States)
Papike, J. J.
(South Dakota School of Mines and Technology Rapid City, SD, United States)
Simon, S. B.
(South Dakota School of Mines and Technology Rapid City, United States)
Shimizu, N.
(MIT Cambridge, MA, United States)
Yurimoto, H.
(Tsukuba, University Japan)
Date Acquired
August 14, 2013
Publication Date
March 1, 1990
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 54
ISSN: 0016-7037
Subject Category
Lunar And Planetary Exploration
Accession Number
90A30849
Funding Number(s)
CONTRACT_GRANT: NAG9-22
Distribution Limits
Public
Copyright
Other

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