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Geochemistry of impact glasses and target rocks from the Zhamanshin Impact Structure, Kazakhstan: Implications for mixing of target and impactor matter

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00025798%3A_____%2F16%3A00000042" target="_blank" >RIV/00025798:_____/16:00000042 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985831:_____/16:00461314 RIV/00216208:11310/16:10328116

  • Result on the web

    <a href="http://www.sciencedirect.com/science/journal/00167037/190" target="_blank" >http://www.sciencedirect.com/science/journal/00167037/190</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.gca.2016.06.031" target="_blank" >10.1016/j.gca.2016.06.031</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Geochemistry of impact glasses and target rocks from the Zhamanshin Impact Structure, Kazakhstan: Implications for mixing of target and impactor matter

  • Original language description

    Internal structure and element chemistry including contents of highly siderophile elements (HSE) and Os isotope ratios have been studied in target rocks and impact glasses of the Zhamanshin impact. They can be subdivided into acidic types (irghizites; 69-76 wt.% SiO2), basic splashforms (53-56 wt.% SiO2), and highly inhomogeneous composites. A comparison with the target rocks shows that zhamanshinites and basic splash-forms have no detectable admixture of the projectile matter. In contrast, irghizites exhibit clear admixture of the projectile, which was incorporated by complex processes accompanied by strong element fractionations. Microscopy confirms that irghizites were formed by coalescence of smaller molten glass droplets sized typically below 1 mm. Irghizites exhibit significant enrichments in Ni, Co and Cr, whose concentrations are locally enriched in the rims of the original small droplets. A portion of these elements and also part of Fe and Mn and other elements were derived from the impactor, most likely a Ni-rich carbonaceous chondrite. The contents of HSE are low and strongly fractionated, with moderate depletions of Pt and Pd and strong depletions of other HSE with respect to chondritic element ratios. Osmium shows the strongest depletion, likely related to the presence of oxygen in the post-impact atmosphere causing strong Os loss through volatilization. The observed structural and microchemical features of irghizites are interpreted to reflect variable proportions of the uppermost target sediments and the projectile matter, with HSE element ratios influenced by evaporation and condensation processes, and differences in volatility of individual HSE elements and/or their compounds. Two possible pathways of incorporation of the projectile matter into the irghizites include either re-condensation of evaporated projectile matter on the surface of glass droplets, or incorporation of less chemically fractionated microparticles dispersed by the explosion.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    DD - Geochemistry

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GA13-22351S" target="_blank" >GA13-22351S: Combined use of novel and traditional stable isotope systems in identifying source components and processes of moldavite formation</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2016

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Geochimica et Cosmochimica Acta

  • ISSN

    0016-7037

  • e-ISSN

  • Volume of the periodical

    190

  • Issue of the periodical within the volume

    1 October

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    26

  • Pages from-to

    239-264

  • UT code for WoS article

    000388802600014

  • EID of the result in the Scopus database