藏南晚白垩世包地花岗岩的成因:岩浆补给和地壳增厚的意义

GSA Bulletin Pub Date : 2023-01-10 DOI:10.1130/b36530.1
Ding-Jun Wen, Xiumian Hu, Jinbiao Yu, Xiaolei Wang, T. Chapman, Rui-Qiang Wang
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引用次数: 0

摘要

含包体花岗岩类的暴露为直接评价弧源岩浆岩的成分变异性与成因深度之间的联系提供了难得的机会。岗底斯基长~ 1000 km,是一种由镁质到长英质组成的复合基;SiO2的范围从51 wt%到70 wt%。冈底斯岩体中尼莫岩体、仁布岩体和日喀则岩体的新锆石U - Pb定年与晚白垩世(约90 ~ 85 Ma)的侵位和结晶一致。岩体基性岩浆包裹体具有低SiO2 (50.9 ~ 56.0% wt%)、低Nb/U、低Ce/Pb、低Nb/La的特征,轻稀土元素和大离子亲石元素富集,高场强元素富集。这些地球化学特征与全岩亏缺εNd(t)(+4.2 ~ +4.7)和锆石εHf(t)(+9.0 ~ +13.8)相结合,表明它们是由与俯冲相关流体相关的亏缺地幔源部分熔融形成的。高SiO2 (55.6% ~ 66.9% wt%)花岗岩具有低Y、Yb含量、高Sr/Y和La/Yb比值的硅质地球化学特征。全岩εNd(t)(+4.0 ~ +5.5)和锆石εHf(t)(+6.9 ~ +14.3)均为正值,且不相容元素富集,表明花岗岩类来源于幼期下地壳的部分熔融作用。地球化学模拟表明,MMEs和埃达克质花岗岩的成分多样性继承自非均质来源。这种成因关系表明,下镀玄武岩岩浆可能提供了足够的热量,引发了增厚地壳的融化,从而形成了包裹体花岗岩。在这方面,弧岩的成因可以反映地壳厚度的演变。研究结果表明,晚白垩世(90 ~ 85 Ma)地壳增厚至50 km,并提供了新生代印亚碰撞前地壳增厚的岩浆记录。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Origin of Late Cretaceous, enclave-bearing granitoids in southern Tibet: Implications for magma recharge and crustal thickening
Exposures of enclave-bearing granitoids can provide rare opportunities to directly evaluate the connection between compositional variability and the depth of origin of arc magmatic rocks. The ∼1000 km long Gangdese batholith is a composite batholith with composition from mafic to felsic; SiO2 ranges from 51 wt% to 70 wt%. New zircon U−Pb dating of the Nyemo plutons, Renbu plutons, and Xigaze plutons in the Gangdese batholith is consistent with their emplacement and crystallization in the Late Cretaceous (ca. 90−85 Ma). Mafic magmatic enclaves (MMEs) in the plutons are characterized by low SiO2 (50.9−56.0 wt%) and Nb/U, Ce/Pb, and Nb/La ratios coupled with enrichment in light rare earth elements and large ion lithophile elements and depletion in high field strength elements. These geochemical features, combined with depleted whole-rock εNd(t) (+4.2 to +4.7) and zircon εHf(t) (+9.0 to +13.8), suggest that they were derived by partial melting of a depleted mantle source associated with subduction-related fluids. The granitoids with high SiO2 (55.6−66.9 wt%) display adakitic geochemical characteristics, such as low Y and Yb contents, and high Sr/Y and La/Yb ratios. Their positive whole-rock εNd(t) (+4.0 to +5.5) and zircon εHf(t) (+6.9 to +14.3) values, as well as enrichment of incompatible elements, indicate that the granitoids were derived from partial melting of the juvenile lower crust. Geochemical modeling suggests that the compositional diversities of MMEs and adakitic granitoids were inherited from heterogeneous sources. This genetic relationship indicates that the underplated basaltic magmas could have supplied sufficient heat to trigger the melting of the thickened crust and thus formation of the enclave-bearing granitoid. In this regard, the origin of arc rocks can mirror the evolution of crustal thickness. Our results reveal that the crust was thickened to ∼50 km during the Late Cretaceous (90−85 Ma) and provide a magmatic record of crustal thickening prior to the Cenozoic Indo-Asia collision.
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