Post-collisional reworking of juvenile mafic lower crust for the petrogenesis of late Triassic adakitic rocks in the East Kunlun Orogen

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Gang Wen , Guo-Chao Sun , Zi-Fu Zhao , Li-Qun Dai , Yao Zhou
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Abstract

The East Kunlun Orogen (EKO), a major component of the Greater Tibetan Plateau, provides an excellent natural laboratory to investigate the tectonic evolution of the Paleo-Tethys Ocean (also known as the A'nyemaqen Ocean in the EKO). We present a combined study of in situ zircon UPb ages and LuHf isotopic compositions, and whole-rock major and trace element and Sr–Nd–Hf isotopic compositions of the post-collisional Xiangjia granodiorite at the eastern end of the EKO. Zircon UPb dating indicates that the Xiangjia granodiorites were emplaced at 225.0–217.1 Ma. Relict zircon cores yield ages of 267.5–239.5 Ma. These granodiorites are calc-alkaline to high-K calc-alkaline and metaluminous to weakly peraluminous, enriched in large-ion lithophile elements and light rare earth elements, and depleted in high field strength elements (e.g., Nb and Ta) and heavy rare earth elements. They yield trace element characteristics that are typical of adakitic rocks, including high Sr (493–590 ppm) and low Yb (0.74–1.12 ppm) and Y (8.83–12.24 ppm) contents, high Sr/Y (40.47–63.64) and (La/Yb)N (11.81–30.91) ratios, and positive Eu anomalies. The UPb ages and Hf isotopic compositions of the relict zircon cores and whole-rock SrNd isotopic compositions of the Xiangjia adakitic rocks are similar to those of the mafic arc magmatic rocks formed during the subduction of the Paleo-Tethys Ocean, suggesting they originated from the reworking of juvenile mafic lower crust. Phase equilibrium modelling suggests that the contemporaneous adakitic rocks from Xiangjia and other areas in the EKO are likely the products of partial melting of the juvenile mafic arc rocks under granulite-facies conditions at 10–11 kbar and 934–951 °C, possibly related to slab break-off in a post-collisional setting.

东昆仑造山带三叠纪晚期黑云母岩石成岩过程中的幼生黑云母下地壳碰撞后再加工问题
东昆仑造山带(EKO)是大青藏高原的主要组成部分,为研究古特提斯洋(EKO中又称阿尼玛卿洋)的构造演化提供了绝佳的天然实验室。我们对东高加索地区东端碰撞后的向家花岗闪长岩进行了原位锆石UPb年龄和LuHf同位素组成,以及全岩主要元素、微量元素和Sr-Nd-Hf同位素组成的综合研究。锆石UPb年代测定表明,向家花岗闪长岩成岩于225.0-217.1Ma。相关锆石岩芯的年代为 267.5-239.5 Ma。这些花岗闪长岩为钙碱性至高K钙碱性、金属铝质至弱过铝质,富含大离子亲岩元素和轻稀土元素,而高场强元素(如Nb和Ta)和重稀土元素则贫乏。它们产生的微量元素特征是典型的英安岩,包括高 Sr(493-590 ppm)、低 Yb(0.74-1.12 ppm)和 Y(8.83-12.24 ppm)含量,高 Sr/Y (40.47-63.64)和 (La/Yb)N (11.81-30.91)比值,以及正 Eu 异常。向家岽岩的残余锆石岩心的UPb年龄和Hf同位素组成以及全岩的SrNd同位素组成与古特提斯洋俯冲过程中形成的黑云质弧岩浆岩相似,表明它们起源于幼年黑云质下地壳的再加工。相平衡模型顯示,向家和東南九龍其他地區的同時代赤鐵岩很可能是幼年黑雲母弧岩在10-11千巴和934-951攝氏度的花崗岩岩相條件下局部熔化的產物,可能與碰撞後的板塊斷裂有關。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Lithos
Lithos 地学-地球化学与地球物理
CiteScore
6.80
自引率
11.40%
发文量
286
审稿时长
3.5 months
期刊介绍: Lithos publishes original research papers on the petrology, geochemistry and petrogenesis of igneous and metamorphic rocks. Papers on mineralogy/mineral physics related to petrology and petrogenetic problems are also welcomed.
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