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Petrogenesis and geodynamic implications of the Late Carboniferous felsic volcanics in the Bogda belt, Chinese Northern Tianshan

机译:天山北部博格达地带晚石炭世长英质火山岩的岩石成因及其地球动力学意义

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An integrated study on petrology and geochemistry has been carried out on the Late Carboniferous I-type felsic volcanics of the Liushugou Formation in the Bogda belt to constrain the late Paleozoic tectonic evolution of the Bogda belt. The felsic volcanics were dated to be 315 to 319 Ma and are composed of trachy-andesite-trachyte ignimbrites and rhyolite lavas. They are in conformable contact with high-Al basalt. The eruption of the felsic volcanics and high-Al basalt is not bimodal volcanism, but is related to bimodal magma (basaltic and rhyolitic magmas). MELTS modeling and comparison with previous basaltic melting experiments indicate that the felsic volcanics are likely produced by partial melting of hydrated mafic crust rather than fractional crystallization of high-Al basalt. It is also supported by relatively large amounts of felsic volcanics to high-Al basalts and remarkably different incompatible element ratios (e.g., Th/Zr, Nb/Zr and U/Zr) of the rocks. The Bogda felsic volcanics have positive epsilon(Nd(t)) values (6.2-7.4), low Pb isotopes and low zircon saturation temperatures, consistent with a derivation from a juvenile crust in an arc setting. The intermediate ignimbrites display melting-mingling textures and abundant feldspar aggregates and have various delta Eu ratios, indicating that magma mingling and feldspar fractionation processes may have played an important role in the genesis of the ignimbrites. In contrast, the Early Permian felsic rocks in this region are of post-collisional A-type. We therefore propose that the Bogda belt was an island arc in the Late Carboniferous and then switched to a post-collisional setting in the Early Permian due to the arc-arc collision at the end of the Late Carboniferous. (C) 2016 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.
机译:对博格达地带柳树沟组晚石炭世I型长英质火山岩进行了岩石学和地球化学的综合研究,以约束博格达地带的晚古生代构造演化。长英质火山的年代为315至319 Ma,由长曲安山岩长曲奇火成岩和流纹岩熔岩组成。它们与高铝玄武岩保持一致的接触。长石质火山岩和高铝玄武岩的喷发不是双峰型火山作用,而是与双峰型岩浆(玄武质和流纹岩浆)有关。 MELTS建模和与之前的玄武岩融化实验的比较表明,长英质火山岩可能是由水合镁铁质地壳的部分融化而不是高Al玄武岩的部分结晶而产生的。相对于高铝玄武岩的大量长生火山和岩石的不相容元素比率(例如Th / Zr,Nb / Zr和U / Zr)明显不同也支持了这一点。博格达长英质火山的ε(Nd(t))值为正值(6.2-7.4),Pb同位素低,锆石饱和温度低,这与弧形环境中的幼年壳相一致。中间的火成岩显示出熔融混合的纹理和丰富的长石聚集体,并具有不同的δEu比,表明岩浆混合和长石的分馏过程可能在火成岩的形成中发挥了重要作用。相反,该地区早二叠世的长英质岩石为碰撞后的A型。因此,我们建议Bogda带是石炭纪晚期的岛状弧,然后由于在石炭纪晚期的弧-弧碰撞而切换到早二叠世的碰撞后环境。 (C)2016国际冈瓦那研究协会。由Elsevier B.V.发布。保留所有权利。

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