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Equilibration temperatures of EL chondrites: A major downward revision in the ferrosilite contents of enstatiteA study of enstatite grains separated from EL6 chondrites shows ferrosilite contents to be approx. 0.02-0.04 mol%, about an order of magnitude lower than reported in the literature. The higher values reported earlier can probably be attributed to the excitation of Fe atoms in Fe-Ni and FeS, in part from micrometer-sized blebs of FeS and Fe-Ni commonly present in enstatite grains but mainly from large neighboring opaque grains excited by bremsstrahlung or by doubly backscattered electrons. Our EL6 ferrosilite contents are similar to those observed in coarse enstatite grains in some aubrites. The equilibrium between ferrosilite and Si-bearing kamacite is highly temperature dependent. At constant Si concentration in kamacite, the equilibrium ferrosilite mole fraction drops by a factor of roughly 2.5 for each 100 K decrease in the equilibrium temperature. As a result, the compositions of these two most common EL6 phases can be used to estimate metamorphic equilibration temperatures. The inferred temperatures are near 1200 K.
Document ID
19950035324
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wasson, John T.
(Univ. of California, Los Angeles, CA United States)
Kallemeyn, Gregory W.
(Univ. of California, Los Angeles, CA United States)
Rubin, Alan E.
(Univ. of California, Los Angeles, CA United States)
Date Acquired
August 16, 2013
Publication Date
September 1, 1994
Publication Information
Publication: Meteoritics
Volume: 29
Issue: 5
ISSN: 0026-1114
Subject Category
Lunar And Planetary Exploration
Accession Number
95A66923
Funding Number(s)
CONTRACT_GRANT: NAGW-3535
Distribution Limits
Public
Copyright
Other

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