Geochemical, thermodynamic and Li isotope constraints on the genesis of rare-metal pegmatites: Implications for crustal Li cycling

IF 4 1区 地球科学 Q1 GEOGRAPHY, PHYSICAL
Qing Du , Jiyuan Yin , Wenjiao Xiao , Tao Wang , Mike Fowler , Zhiyong Zhu , Zaili Tao , Guibin Zhang , Min Sun , Guochun Zhao
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引用次数: 0

Abstract

Rare-metal pegmatite deposits are widespread in collisional settings around the world and are increasingly important to the global requirement for critical metals. However, their genesis and rare-metal enrichment processes remain enigmatic, particularly concerning whether they originate from highly fractionated granitic magmas or anatexis of metasedimentary rocks. In this study, we integrate zircon UPb geochronology, whole-rock and mineral chemistry and Li isotopic compositions of pegmatites and associated granitoids from the West Kunlun Orogenic Belt (WKOB) in northern Tibetan Plateau, to investigate these issues. Zircon UPb dating yields weighted mean ages of 223 Ma for the pegmatites and 213–222 Ma for the adjacent granitoids. Compared with the granitoids, the pegmatites exhibit distinct geochemical signatures, including high SiO2 (72.9–74.5 wt%) and Al2O3 (16.2–17.2 wt%), low TiO2 (<0.01 wt%), TFe2O3 (0.09–0.21 wt%) and MgO (<0.02 wt%), and strongly peraluminous signatures (A/CNK = 1.04–2.56). δ7Li values of Li-rich pegmatites and Li-poor pegmatites are relatively uniform (+2.11 to +0.8 ‰), but for muscovite the δ7Li values extend to lower values in Li-poor than Li-rich pegmatites (−2.93 to +2.11 ‰ and + 0.37 to +2.98 ‰, respectively). The absence of coherent fractionation trends between pegmatites and granitoids (e.g., Rb, Cs), along with a lack of mineralogical evidence for extreme magmatic differentiation, argues against a fractionated granite origin. Instead, Li isotope models of partial melting, thermodynamically-defined phase equilibria and associated elemental calculations all demonstrate that the West Kunlun Li-rich pegmatites were likely generated by melting of Li-rich claystone under amphibolite facies conditions, whereas the Li-poor pegmatites originated from typical metasedimentary sources. We propose that the involvement of Li-rich claystone into the middle to lower crust during collisional orogenesis was a key control on the formation of Li-rich pegmatites in the WKOB. This mechanism highlights the metallogenic significance of crustal-scale Li cycling and may be broadly applicable to rare metal pegmatite systems in other collisional orogenic belts.
稀土伟晶岩成因的地球化学、热力学和Li同位素约束:地壳Li循环的意义
稀有金属伟晶岩矿床在世界各地的碰撞环境中广泛存在,对全球对关键金属的需求越来越重要。然而,它们的成因和稀有金属的富集过程仍然是一个谜,特别是它们是来自高分馏的花岗质岩浆还是变质沉积岩的深熔。锆石UPb定年得到伟晶岩的加权平均年龄为223 Ma,相邻花岗岩的加权平均年龄为213-222 Ma。与花岗岩类相比,伟晶岩具有明显的地球化学特征,高SiO2(72.9 ~ 74.5 wt%)和Al2O3(16.2 ~ 17.2 wt%),低TiO2 (<0.01 wt%)、TFe2O3(0.09 ~ 0.21 wt%)和MgO (<0.02 wt%),强过铝特征(A/CNK = 1.04 ~ 2.56)。富锂伟晶岩和贫锂伟晶岩的δ7Li值相对均匀(+2.11 ~ +0.8 ‰),而白云母贫锂伟晶岩的δ7Li值较富锂伟晶岩的δ7Li值低(分别为- 2.93 ~ +2.11 ‰和 + 0.37 ~ +2.98 ‰)。伟晶岩和花岗岩类(如Rb、Cs)之间缺乏一致的分选趋势,以及缺乏极端岩浆分选的矿物学证据,这些都反对分选花岗岩的起源。相反,部分熔融的锂同位素模型、热力学定义的相平衡以及相关的元素计算都表明,西昆仑富锂伟晶岩可能是在角闪岩相条件下由富锂粘土岩熔融形成的,而贫锂伟晶岩则来自典型的变质沉积岩。我们认为,在碰撞造山过程中,富锂粘土岩进入中下地壳是控制WKOB富锂伟晶岩形成的关键因素。这一机制突出了地壳尺度上Li旋回的成矿意义,可广泛应用于其他碰撞造山带的稀有金属伟晶岩系统。
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来源期刊
Global and Planetary Change
Global and Planetary Change 地学天文-地球科学综合
CiteScore
7.40
自引率
10.30%
发文量
226
审稿时长
63 days
期刊介绍: The objective of the journal Global and Planetary Change is to provide a multi-disciplinary overview of the processes taking place in the Earth System and involved in planetary change over time. The journal focuses on records of the past and current state of the earth system, and future scenarios , and their link to global environmental change. Regional or process-oriented studies are welcome if they discuss global implications. Topics include, but are not limited to, changes in the dynamics and composition of the atmosphere, oceans and cryosphere, as well as climate change, sea level variation, observations/modelling of Earth processes from deep to (near-)surface and their coupling, global ecology, biogeography and the resilience/thresholds in ecosystems. Key criteria for the consideration of manuscripts are (a) the relevance for the global scientific community and/or (b) the wider implications for global scale problems, preferably combined with (c) having a significance beyond a single discipline. A clear focus on key processes associated with planetary scale change is strongly encouraged. Manuscripts can be submitted as either research contributions or as a review article. Every effort should be made towards the presentation of research outcomes in an understandable way for a broad readership.
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