首页> 外文会议>Seventh Biennial SGA Meeting Vol.2 Aug 24-28, 2003 Athens/Greece >The age of formation of a marble in the Moldanubian Varied Group, Bohemian massif, Czech Republic using Re-Os dating of molybdenite
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The age of formation of a marble in the Moldanubian Varied Group, Bohemian massif, Czech Republic using Re-Os dating of molybdenite

机译:捷克共和国波希米亚地块摩尔达努比亚变质组中大理石的形成年龄,使用的是辉钼矿的Re-Os定年法

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A Re-Os geochronological investigation was undertaken on sparsely disseminated molybdenite occurring in a regionally metamorphosed carbonatite-like marble, which belongs to the crystalline sequence of the Moldanubian Varied Group. The mineralogical composition of the marble is complex and includes a Mo-Th-Nb-REE mineralization that is concentrated in silicate-rich horizons with a high component of alkaline volcanic-sedimentary detrital material. These mineralized horizons form a continuous layer that is present only in rocks underlying graphite bed. We suggest that a component of the mineralization may arise from me-tasomatic infiltration into more porous detrital horizons within the carbonatite-like marbles during regional metamorphism. The overlying sequence containing organic-rich units may have contributed Mo-Th to the mineralization, but we do not exclude the possibility that these components could have come from the hosting alkaline volcanic-sedimentary material, where Nb and REE may have been enriched. The confluence of both a porous medium and available ore components may have focused metal-enriched metamorphic fluids. We suggest that the Re-Os age of the molybdenite records regional amphibolite grade metamorphism at about 495 Ma in the southern Bohemian massif. Because the Re-Os chronometer in molybdenite is demonstrably robust through granulite facies metamorphism, it is not affected by subsequent thermal overprints associated with the Variscan orogeny, and preserves an important part of the Cadomian event in this region.
机译:进行了一次Re-Os地质年代学调查,研究了一种稀疏散布的辉钼矿,该辉钼矿发生在区域变质的类碳酸盐岩样大理石中,属于大理石结晶变种。大理石的矿物学组成很复杂,并且包括Mo-Th-Nb-REE矿化作用,该矿化作用富集于富含硅酸盐的地层中,具有高含量的碱性火山沉积碎屑物质。这些矿化的层位形成一个连续层,仅存在于石墨床下面的岩石中。我们建议在区域变质过程中,碳酸盐岩状大理石内的介孔渗入更多的多孔碎屑地层中,可能是矿化的一部分。上层序列中富含有机物的单元可能对矿化作用贡献了Mo-Th,但我们不排除这些组分可能来自宿主碱性火山沉积物质的可能性,在这些沉积物中,Nb和REE可能已经富集。多孔介质和可利用的矿石成分的汇合处可能具有富集的富集金属的变质流体。我们认为辉钼矿的Re-Os年龄记录了波西米亚南部断层的大约495 Ma的区域闪石级变质作用。由于辉钼矿中的Re-Os计时码表通过粒岩相变质作用表现出明显的鲁棒性,因此不受随后与Variscan造山运动有关的热套印的影响,并且保留了该地区Cadomian事件的重要部分。

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