Olivine zoning and retrograde olivine-orthopyroxene-metal equilibration in H5 and H6 chondrites
dc.contributor.author | Reisener, R. J. | |
dc.contributor.author | Goldstein, J. I. | |
dc.contributor.author | Petaev, M. I. | |
dc.date.accessioned | 2021-02-12T21:41:09Z | |
dc.date.available | 2021-02-12T21:41:09Z | |
dc.date.issued | 2006-01-01 | |
dc.identifier.citation | Reisener, 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.issn | 1945-5100 | |
dc.identifier.doi | 10.1111/j.1945-5100.2006.tb00455.x | |
dc.identifier.uri | http://hdl.handle.net/10150/656218 | |
dc.description.abstract | Electron 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.iso | en | |
dc.publisher | The Meteoritical Society | |
dc.relation.url | https://meteoritical.org/ | |
dc.rights | Copyright © The Meteoritical Society | |
dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | |
dc.subject | Taenite | |
dc.subject | metal | |
dc.subject | pyroxenes | |
dc.subject | olivine | |
dc.title | Olivine zoning and retrograde olivine-orthopyroxene-metal equilibration in H5 and H6 chondrites | |
dc.type | Article | |
dc.type | text | |
dc.identifier.journal | Meteoritics & Planetary Science | |
dc.description.collectioninformation | The 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.version | Final published version | |
dc.description.admin-note | Migrated from OJS platform February 2021 | |
dc.source.volume | 41 | |
dc.source.issue | 12 | |
dc.source.beginpage | 1839 | |
dc.source.endpage | 1852 | |
refterms.dateFOA | 2021-02-12T21:41:09Z |