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    Iron oxidation state in impact glass from the K/T boundary at Beloc, Haiti, by high-resolution XANES spectroscopy

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    Author
    Giuli, Gabriele
    Eeckhout, Sigrid Griet
    Paris, Eleonora
    Koeberl, Christian
    Pratesi, Giovanni
    Issue Date
    2005-01-01
    Keywords
    Chicxulub Impact crater
    impact glasses
    K/T boundary
    Xanes
    
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    Citation
    Giuli, 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.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656687
    DOI
    10.1111/j.1945-5100.2005.tb00132.x
    Additional Links
    https://meteoritical.org/
    Abstract
    We 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.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2005.tb00132.x
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    Meteoritics & Planetary Science, Volume 40, Number 11 (2005)

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