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dc.contributor.authorGiuli, Gabriele
dc.contributor.authorEeckhout, Sigrid Griet
dc.contributor.authorParis, Eleonora
dc.contributor.authorKoeberl, Christian
dc.contributor.authorPratesi, Giovanni
dc.date.accessioned2021-02-12T22:54:18Z
dc.date.available2021-02-12T22:54:18Z
dc.date.issued2005-01-01
dc.identifier.citationGiuli, G., Eeckhout, S. G., Paris, E., Koeberl, C., & Pratesi, G. (2005). Iron oxidation state in impact glass from the K/T boundary at Beloc, Haiti, by high‐resolution XANES spectroscopy. Meteoritics & Planetary Science, 40(11), 1575-1580.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2005.tb00132.x
dc.identifier.urihttp://hdl.handle.net/10150/656687
dc.description.abstractWe examined the local iron environment in nine impact glasses from the Cretaceous- Tertiary (K/T) boundary section at Beloc, Haiti, which formed as the result of impact melting during the Chicxulub impact event. The samples have been analyzed by Fe K-edge high-resolution X-ray absorption near edge structure (XANES) spectroscopy to obtain data on both the Fe oxidation state and the coordination number. The pre-edge peak of our high-resolution XANES spectra display noticeable variations indicative of significant changes in the Fe oxidation state spanning a wide range from about 20 to 75 mol% trivalent Fe. All data plot along the same trend, falling between two mixing lines joining a point calculated as the mean of a group of tektites studied so far (consisting of four- and five-coordinated Fe2+) to [4]Fe^(3+) and [5]Fe^(3+), respectively. Thus, the XANES spectra can be interpreted as a mixture of [4]Fe^(2+), [5]Fe^(2+), [4]Fe^(3+), and [5]Fe^(3+). There is no evidence for six-fold coordinated Fe; however, its presence in small amounts cannot be excluded from XANES data alone. Our observations can be explained by two possible scenarios: either these impact glasses formed under very reducing conditions and, because of their small size, were easily oxidized in air while still molten, or they formed under a variety of different oxygen fugacities resulting in different Fe oxidation states. In the first case, the oxidation state and coordination number would imply similar formation conditions as splash-form tektites, followed by progressive oxidation.
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.subjectChicxulub Impact crater
dc.subjectimpact glasses
dc.subjectK/T boundary
dc.subjectXanes
dc.titleIron oxidation state in impact glass from the K/T boundary at Beloc, Haiti, by high-resolution XANES spectroscopy
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.volume40
dc.source.issue11
dc.source.beginpage1575
dc.source.endpage1580
refterms.dateFOA2021-02-12T22:54:18Z


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