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首页> 外文期刊>Contributions to Mineralogy and Petrology >The Skien lavas, Oslo Rift: petrological disequilibrium and geochemical evolution
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The Skien lavas, Oslo Rift: petrological disequilibrium and geochemical evolution

机译:奥斯陆裂谷的斯基恩熔岩:​​岩石学不平衡和地球化学演化

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The Skien lavas, which form the earliest phase of basaltic magmatism within the Permo-Carboniferous Oslo Rift, contain multiple generations of clinopyroxene which exhibit strong petrological and geochemical disequilibrium. Three principal core compositions have been identified: (1) low-jadeite, high-Mg, Cr-diopside cores (CrMgDi) with strongly depleted trace-element signatures, which are believed to be xenocrystic in origin; (2) Mg-rich, Cr-poor diopside cores (MgDi) with moderately depleted trace-element signatures which probably represent early cognate growth; and (3) more dominant, low-Mg, phenocrystic diopside cores (PhenDi). Several samples contain CrMgDi or MgDi cores which have been subjected to resorption and partial re-equilibration with their host melts, indicative of extensive disequilibrium and magma mixing. These three core types are overgrown by trace-element-enriched Ti-augite, which also forms megacrysts and late-stage lava groundmass. Calculated Ti-augite/melt partition coefficients show clinopyroxene compatibility of the M-HREE, Zr, Hf and Y. The LILE, Sr, and Nb remain incompatible. εSr300 and εNd300 of Ti-augite overgrowths, phenocrystic diopside, and MgDi diopside cores show that intrasample isotopic disequilibrium existed when the host basalts were erupted. All epsilon values lie within the range of data previously published for the Skien lavas. Detailed examination of the chemical, isotopic and textural disequilibrium features seen in these lavas has enabled us to place constraints upon the magmatic evolution of this basalt suite, ranging from xenocryst incorporation to cognate multistage pyroxene growth, as well as identifying clear evidence of magma mixing and possible crustal contamination.
机译:Skien熔岩形成了Permo-Carboniferous Oslo裂谷内玄武岩浆作用的最早阶段,包含多代次生的次氯环戊二烯,表现出强烈的岩石学和地球化学不平衡。已经确定了三个主要的核心成分:(1)具有痕量元素特征强烈耗尽的低硬玉石,高镁,Cr透辉石核(CrMgDi),据信其起源是异晶的; (2)富含镁,贫铬的透辉石核(MgDi),其痕量元素特征适度耗尽,可能代表早期同源生长; (3)占主导地位的低镁,单晶透辉石核(PhenDi)。几个样品含有CrMgDi或MgDi核,这些核已通过其主体熔体进行了吸收和部分再平衡,表明存在广泛的不平衡和岩浆混合。富含微量元素的钛金铁矿长满了这三种核心类型,钛金铁矿也形成了巨晶和后期熔岩地基。计算得出的钛金铁矿/熔体分配系数显示M-HREE,Zr,Hf和Y的斜辉石相容性。LILE,Sr和Nb保持不相容。钛金长生岩,透辉石透辉石和MgDi透辉石岩芯的εSr300和εNd300表明,当宿主玄武岩爆发时,存在样品内同位素不平衡。所有epsilon值都在先前为Skien熔岩发布的数据范围内。对这些熔岩中所见化学,同位素和质地不平衡特征的详细检查,使我们能够对这一玄武岩组的岩浆演化施加约束,从掺入异晶相到同源多级辉石生长,以及识别岩浆混合和形成的清晰证据。可能的地壳污染。

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  • 来源
    《Contributions to Mineralogy and Petrology 》 |2001年第6期| 701-719| 共19页
  • 作者单位

    Mineralogisk-Geologisk Museum Sars'gate 1 0562 Oslo Norway;

    Department of Geology Universitetet i Oslo Postboks 1047 Blindern 0316 Oslo Norway;

    PRIS University of Reading P.O. Box 227 Whiteknights Reading Berks UK;

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