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Petrographic studies of refractory inclusions from the Murchison meteoriteTextural and mineral-chemical data on freeze-thaw disaggregated refractory inclusions from the Murchison meteorite are reported. The data were obtained with neutron activation analysis, SEM, and spectroscopy, the study revealed corundum-bearing inclusions, spinel-hibonite aggregates and spherules, and spinel-pyroxene and elivine-pyroxene inclusions. One of the three spinel-, pyroxene-, forsterite-rich inclusions had an amoeba-shaped spinel-pyroxene core, implying vapor-to-solid condensation and therefore crystallization from a melt. It is concluded that the meteorite formation encompassed diverse nebular materials, and that further studies of the meteorite will enhance the data base on the planetary nebular processes.
Document ID
19850035523
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Macpherson, G. J.
(Smithsonian Institution, Washington, DC; Chicago, University Chicago, IL, United States)
Grossman, L.
(Smithsonian Institution Washington, DC, United States)
Hashimoto, A.
(Chicago, University Chicago, IL, United States)
Bar-Matthews, M.
(Geological Survey of Israel, Jerusalem, Israel; Chicago, University Chicago, IL, United States)
Tanaka, T.
(Geological Survey of Japan, Yatabe, Ibaraki, Japan; Chicago, University Chicago, IL, United States)
Date Acquired
August 12, 2013
Publication Date
November 15, 1984
Publication Information
Publication: Journal of Geophysical Research, Supplement
Volume: 89
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
85A17674
Funding Number(s)
CONTRACT_GRANT: NSF EAR-82-18154
CONTRACT_GRANT: NAG9-54
CONTRACT_GRANT: NGR-14-001-249
Distribution Limits
Public
Copyright
Other

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