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首页> 外文期刊>Journal of Asian earth sciences >Crustal thickening prior to 220 Ma in the East Kunlun Orogenic Belt: Insights from the Late Triassic granitoids in the Xiao-Nuomuhong pluton
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Crustal thickening prior to 220 Ma in the East Kunlun Orogenic Belt: Insights from the Late Triassic granitoids in the Xiao-Nuomuhong pluton

机译:东昆仑造山带220 Ma之前的地壳增厚:从小诺木洪岩体的晚三叠世花岗质体中获得的见解

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摘要

The East Kunlun Orogenic Belt (EKOB) played an important role in plate tectonics, magma generation, and crustal evolution. Late Triassic granodiorites and their mafic micro-granular enclaves (MMEs) from Xiao-Nuomuhong in the EKOB were studied for geochemistry and geochronology to constrain their pet-rogenesis. Zircon LA-ICP-MS dating indicates that the Xiao-Nuomuhong granodiorites are coeval with their MMEs (~222 Ma). The granodiorites are high-K calc-alkaline rocks that are enriched in Rb, Th, U and LREE, and depleted in Cr, Ni and HFSE, with high Sr/Y ratios (82.2-85.3) and geochemically resemble the lower crust-derived adakites. The MMEs are also high-K calc-alkaline rocks, with high Al_2O_3 (16.8-18.8 wt.%), low Mg~# (30-40), Nb, Zr and Hf, with weak negative Eu anomalies (Eu/Eu~# = 0.8-0.9). We suggest the MMEs are mafic magmatic globules that were injected into the felsic host magma. The adak-itic rocks from the Xiao-Nuomuhong pluton were generated by partial melting of thickened crust, while the primitive compositions of the MMEs were most likely from the lithospheric mantle beneath the EKOB. The Late Triassic Xiao-Nuomuhong pluton is important evidence that crustal thickening in the EKOB occurred prior to 220 Ma. The pluton is interpreted as the result of mixing between thickened lower crust-derived melts and lithospheric mantle-derived mafic melts and the protracted magmatic response to the break-off of the Paleo-Tethys oceanic slab at ~232 Ma.
机译:东昆仑造山带(EKOB)在板块构造,岩浆生成和地壳演化中起着重要作用。研究了三叠纪晚期三叠纪花岗闪长岩及其来自EKOB的Xiao-Nuomuhong的镁铁质微颗粒飞地,进行了地球化学和地球年代学研究,以限制它们的成岩作用。 Zircon LA-ICP-MS测年表明,肖诺木洪花岗闪长岩与其MME(〜222 Ma)同生。花岗闪长岩是高K钙碱性岩石,富含Rb,Th,U和LREE,贫Cr,Ni和HFSE,具有高Sr / Y比(82.2-85.3),并且在地球化学上类似于下地壳阿达克人。 MMEs也是高K的钙碱性岩石,具有高Al_2O_3(16.8-18.8 wt。%),低Mg〜#(30-40),Nb,Zr和Hf,负Eu异常弱(Eu / Eu〜 #= 0.8-0.9)。我们建议MME是注入到长英质岩浆中的镁铁质岩浆小球。小诺木洪岩体的Adakitic岩石是由增厚的地壳部分熔融而产生的,而MMEs的原始成分很可能来自于EKOB下方的岩石圈地幔。晚三叠世肖诺木洪岩体是重要的证据,表明EKOB中的地壳增厚发生在220 Ma之前。岩体的解释是厚的下地壳衍生的熔体与岩石圈地幔的镁铁质熔体之间的混合以及对古特提斯洋板在〜232 Ma破裂的持久岩浆反应的结果。

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  • 来源
    《Journal of Asian earth sciences》 |2014年第15期|193-210|共18页
  • 作者单位

    State Key Laboratory of Geological Processes and Mineral Resources, China University of Geosciences, Beijing 100083, China,Gold Geological Institute of CAPF, Langfang 065000, China;

    State Key Laboratory of Geological Processes and Mineral Resources, China University of Geosciences, No. 29, Xueyuan Road, Beijing 100083, China;

    State Key Laboratory of Geological Processes and Mineral Resources, China University of Geosciences, Beijing 100083, China;

    School of Earth and Environmental Sciences, James Cook University, Townsville 4811, Queensland, Australia;

    Gold Geological Institute of CAPF, Langfang 065000, China;

    State Key Laboratory of Geological Processes and Mineral Resources, China University of Geosciences, Beijing 100083, China,Gold Geological Institute of CAPF, Langfang 065000, China;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Geochronology; Geochemistry; Adakite; Mafic microgranular enclave; Paleo-Tethys; East Kunlun;

    机译:地球年代学;地球化学;ak石镁铁质微颗粒飞地;古特提斯东昆仑;

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