大陆深俯冲期间壳幔相互作用:来自东昆仑造山带碰撞后基性火成岩轻Mo同位素的证据

IF 3 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Qing-Chen Yang, Wei Fang, Li-Qun Dai, Li-Tao Ma, Zi-Fu Zhao
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引用次数: 0

摘要

在大陆俯冲带,壳幔相互作用是否会发生以及如何发生,是一个有趣的问题。本文报道了东昆仑造山带晚古生代基性火成岩的锆石U-Pb年龄、Hf同位素、主微量元素和Sr-Nd-Mo同位素。锆石U-Pb测年结果显示,这些岩石的年龄在384-387 Ma之间,与EKO的碰撞后岩浆活动相一致。基性岩的微量元素呈弧型分布,Sr-Nd同位素呈微富集,表明其来源于有地壳物质参与的肥沃地幔。它们的高Th/La比值(0.28 ~ 0.77)与典型洋壳的再循环不一致,但可能与地壳深熔过程中残留的陆壳熔体有关。这些基性岩和片麻岩在Sr-Nd同位素和锆石Hf同位素上的相似性进一步加强了这一点,这些片麻岩代表了EKO的古代大陆地壳成分。值得注意的是,碰撞后基性岩石的δ98Mo值在−0.64‰~−0.07‰之间变化较大。结合富Sr-Nd同位素和高Th/La特征,推测其轻Mo同位素特征继承自深俯冲大陆地壳。考虑到大陆地壳普遍具有较高的δ98Mo值(0.10 ~ 0.40‰)的特征,基性岩石的轻Mo同位素组成应继承于以前大陆地壳衍生熔融体的脱水。研究表明,轻Mo同位素特征可以用来解释碰撞造山带大陆地壳的再循环。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Crust-Mantle Interaction During Continental Deep Subduction: Evidence From Light Mo Isotopes in Post-Collisional Mafic Igneous Rocks From the East Kunlun Orogen

Crust-Mantle Interaction During Continental Deep Subduction: Evidence From Light Mo Isotopes in Post-Collisional Mafic Igneous Rocks From the East Kunlun Orogen

Crust-Mantle Interaction During Continental Deep Subduction: Evidence From Light Mo Isotopes in Post-Collisional Mafic Igneous Rocks From the East Kunlun Orogen

Crust-Mantle Interaction During Continental Deep Subduction: Evidence From Light Mo Isotopes in Post-Collisional Mafic Igneous Rocks From the East Kunlun Orogen

It is intriguing whether and how crust-mantle interaction would proceed in continental subduction zones. Here, we report zircon U-Pb ages and Hf isotopes, major and trace elements, and Sr-Nd-Mo isotopes for Late Paleozoic mafic igneous rocks from the East Kunlun orogen (EKO). Zircon U–Pb dating of these rocks yields concordant ages of 384–387 Ma, corresponding to post-collisional magmatism in the EKO. The mafic rocks are characterized by arc-type trace element distribution patterns and slightly enriched Sr-Nd isotopes, indicating their derivation from a fertile mantle source with the involvement of crustal material. Their high Th/La ratios (0.28–0.77) are inconsistent with the recycling of typical oceanic crust but can be related to continental crust-derived melts with residual allanite during crustal anatexis. This is further strengthened by the similarity in Sr-Nd isotopes and zircon Hf isotopes between these mafic rocks and gneiss that represent ancient continental crustal components in the EKO. Notably, the post-collisional mafic rocks have variably low δ98Mo values of −0.64‰ to −0.07‰. Combined with the enriched Sr-Nd isotopes and high Th/La features, it is inferred that the light Mo isotopic signatures are inherited from the deeply subducted continental crust. Given that continental crust is generally characterized by high δ98Mo values of 0.10–0.40‰, the light Mo isotope compositions of the mafic rocks should be inherited from the previously dehydrated continental crust-derived melts. Our study highlights that the light Mo isotope features can be used to decipher the recycling of continental crust in collisional orogens.

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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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