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Petrological, Geochemical and Sr–Nd–O Isotopic Constraints on the Origin of Garnet and Spinel Pyroxenites from the Moldanubian Zone of the Bohemian Massif

Identifikátory výsledku

  • Kód výsledku v IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985831%3A_____%2F16%3A00460854" target="_blank" >RIV/67985831:_____/16:00460854 - isvavai.cz</a>

  • Nalezeny alternativní kódy

    RIV/00216208:11310/16:10331684

  • Výsledek na webu

    <a href="http://dx.doi.org/10.1093/petrology/egw025" target="_blank" >http://dx.doi.org/10.1093/petrology/egw025</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/petrology/egw025" target="_blank" >10.1093/petrology/egw025</a>

Alternativní jazyky

  • Jazyk výsledku

    angličtina

  • Název v původním jazyce

    Petrological, Geochemical and Sr–Nd–O Isotopic Constraints on the Origin of Garnet and Spinel Pyroxenites from the Moldanubian Zone of the Bohemian Massif

  • Popis výsledku v původním jazyce

    Garnet pyroxenites, spinel pyroxenites, and eclogites in the Moldanubian Zone of the Bohemian Massif form layers and lenses in mantle-derived peridotites that are enclosed by migmatitic gneisses and granulites. We have analysed major and trace elements, and Sr, Nd and oxygen isotopes for a suite of pyroxenites, which vary in composition and origin, from nine localities (Bečváry, Horní Bory, Drahonín, Níhov, Mohelno, Nové Dvory, Horní Kounice, Karlstetten and Meidling-im-Tal) in the Gföhl Unit and Kutná Hora Complex. Based on conventional geothermobarometry, most pyroxenites yield a restricted range of temperatures (∼875–975 °C) over a wide span of pressures (∼10–30 GPa). The pyroxenite suite exhibits large variations in elemental and isotopic compositions, reflecting its complex origin and evolution. Based on the rare earth element (REE) compositions of clinopyroxene (Cpx), three types ( Type A–C) of pyroxenite can be distinguished. Such REE patterns reflect derivation of the melts from depleted (Type A) and enriched (Types B and C) mantle sources. Pyroxenites from eight localities originated as high-pressure crystal cumulates from transient basaltic melts migrating through the lithospheric mantle. In contrast, pyroxenites at the Bečváry locality represent fragments of metamorphosed gabbroic cumulates from oceanic crust. For the pyroxenite suite as a whole, a positive correlation between Sr/Nd and Eu/Eu*, radiogenic 87Sr/86Sr and negative εNd values in clinopyroxene, and variable δ18O values in coexisting garnet argue for the presence of a crustal component in the parental pyroxenite melts. Variations in compatible elements (Ni, Sc, and Co) indicate that combined assimilation and fractional crystallization was important in the evolution of most of the pyroxenite parental melts, although fractional crystallization alone is recorded by the fragments of oceanic crust, perhaps reflecting their pre-subduction crystallization history.

  • Název v anglickém jazyce

    Petrological, Geochemical and Sr–Nd–O Isotopic Constraints on the Origin of Garnet and Spinel Pyroxenites from the Moldanubian Zone of the Bohemian Massif

  • Popis výsledku anglicky

    Garnet pyroxenites, spinel pyroxenites, and eclogites in the Moldanubian Zone of the Bohemian Massif form layers and lenses in mantle-derived peridotites that are enclosed by migmatitic gneisses and granulites. We have analysed major and trace elements, and Sr, Nd and oxygen isotopes for a suite of pyroxenites, which vary in composition and origin, from nine localities (Bečváry, Horní Bory, Drahonín, Níhov, Mohelno, Nové Dvory, Horní Kounice, Karlstetten and Meidling-im-Tal) in the Gföhl Unit and Kutná Hora Complex. Based on conventional geothermobarometry, most pyroxenites yield a restricted range of temperatures (∼875–975 °C) over a wide span of pressures (∼10–30 GPa). The pyroxenite suite exhibits large variations in elemental and isotopic compositions, reflecting its complex origin and evolution. Based on the rare earth element (REE) compositions of clinopyroxene (Cpx), three types ( Type A–C) of pyroxenite can be distinguished. Such REE patterns reflect derivation of the melts from depleted (Type A) and enriched (Types B and C) mantle sources. Pyroxenites from eight localities originated as high-pressure crystal cumulates from transient basaltic melts migrating through the lithospheric mantle. In contrast, pyroxenites at the Bečváry locality represent fragments of metamorphosed gabbroic cumulates from oceanic crust. For the pyroxenite suite as a whole, a positive correlation between Sr/Nd and Eu/Eu*, radiogenic 87Sr/86Sr and negative εNd values in clinopyroxene, and variable δ18O values in coexisting garnet argue for the presence of a crustal component in the parental pyroxenite melts. Variations in compatible elements (Ni, Sc, and Co) indicate that combined assimilation and fractional crystallization was important in the evolution of most of the pyroxenite parental melts, although fractional crystallization alone is recorded by the fragments of oceanic crust, perhaps reflecting their pre-subduction crystallization history.

Klasifikace

  • Druh

    J<sub>x</sub> - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

  • CEP obor

    DD - Geochemie

  • OECD FORD obor

Návaznosti výsledku

  • Projekt

  • Návaznosti

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Ostatní

  • Rok uplatnění

    2016

  • Kód důvěrnosti údajů

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

Údaje specifické pro druh výsledku

  • Název periodika

    Journal of Petrology

  • ISSN

    0022-3530

  • e-ISSN

  • Svazek periodika

    57

  • Číslo periodika v rámci svazku

    5

  • Stát vydavatele periodika

    GB - Spojené království Velké Británie a Severního Irska

  • Počet stran výsledku

    24

  • Strana od-do

    897-920

  • Kód UT WoS článku

    000380254200003

  • EID výsledku v databázi Scopus

    2-s2.0-84978680796