OLIVINE ZONING AND RETROGRADE OLIVINE-ORTHOPYROXENE-METAL EQUILIBRATION IN H5 AND H6 CHONDRITES
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dc.contributor.author | Reisener R.J. | |
dc.contributor.author | Goldstein J.I. | |
dc.contributor.author | Petaev M.I. | |
dc.date.accessioned | 2025-01-04T06:13:57Z | |
dc.date.available | 2025-01-04T06:13:57Z | |
dc.date.issued | 2006 | |
dc.identifier | https://www.elibrary.ru/item.asp?id=13842097 | |
dc.identifier.citation | Meteoritics and Planetary Science, 2006, 41, 12, 1839-1852 | |
dc.identifier.issn | 1086-9379 | |
dc.identifier.uri | https://repository.geologyscience.ru/handle/123456789/47262 | |
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 °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 °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. © The Meteoritical Society, 2006. | |
dc.title | OLIVINE ZONING AND RETROGRADE OLIVINE-ORTHOPYROXENE-METAL EQUILIBRATION IN H5 AND H6 CHONDRITES | |
dc.type | Статья | |
dc.identifier.doi | 10.1111/j.1945-5100.2006.tb00455.x |
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