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dc.contributor.authorReisener, R. J.
dc.contributor.authorGoldstein, J. I.
dc.contributor.authorPetaev, M. I.
dc.date.accessioned2021-02-12T21:41:09Z
dc.date.available2021-02-12T21:41:09Z
dc.date.issued2006-01-01
dc.identifier.citationReisener, R. J., Goldstein, J. I., & Petaev, M. I. (2006). Olivine zoning and retrograde olivine‐orthopyroxene‐metal equilibration in H5 and H6 chondrites. Meteoritics & Planetary Science, 41(12), 1839-1852.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2006.tb00455.x
dc.identifier.urihttp://hdl.handle.net/10150/656218
dc.description.abstractElectron microprobe studies of several H5 and H6 chondrites reveal that olivine crystals exhibit systematic Fe-Mg zoning near olivine-metal interfaces. Olivine Fa concentrations decrease by up to 2 mol% toward zoned taenite + kamacite particles (formed after relatively small amounts of taenite undercooling) and increase by up to 2 mol% toward zoneless plessite particles (formed after ~200 degrees C of taenite undercooling). The olivine zoning can be understood in terms of localized olivine-orthopyroxene-metal reactions during cooling from the peak metamorphic temperature. The silicate-metal reactions were influenced by solid-state metal phase transformations, and the two types of olivine zoning profiles resulted from variable amounts of taenite undercooling at temperatures <700 degrees C. The relevant silicate-metal reactions are modeled using chemical thermodynamics. Systematic olivine Fe-Mg zoning adjacent to metal is an expected consequence of retrograde silicate-metal reactions, and the presence of such zoning provides strong evidence that the silicate and metallic minerals evolved in situ during cooling from the peak metamorphic temperature.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectTaenite
dc.subjectmetal
dc.subjectpyroxenes
dc.subjectolivine
dc.titleOlivine zoning and retrograde olivine-orthopyroxene-metal equilibration in H5 and H6 chondrites
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume41
dc.source.issue12
dc.source.beginpage1839
dc.source.endpage1852
refterms.dateFOA2021-02-12T21:41:09Z


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