岩浆-热液矿床中与矿有关的花岗岩和矿石的锌同位素变化

IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Youqiang Qi, Ruizhong Hu, Haifeng Fan, Jun-Hong Zhao
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引用次数: 0

摘要

金属同位素是研究成矿元素迁移和分布的有力工具。锌(Zn)在流体中主要以氯络合物的形式运输,其价态相对不受氧化还原条件的影响,因此锌同位素可以为岩浆-热液矿床的形成提供有价值的见解。然而,在岩浆-热液系统中,硅熔体中热液流体的析出和含锌矿物的结晶过程中,锌同位素分馏存在显著的不确定性。冷水坑银铅锌矿床是华南地区最大的岩浆热液银矿床之一,与中生代花岗岩浆作用有关,是研究花岗岩浆作用和热液成矿过程中锌同位素变化的理想天然实验室。对热液含锌矿石、脉石矿物、矿相关及非矿相关英质岩进行了系统的锌同位素分析。闪锌矿为主要矿石矿物,根据“黄铜矿病”结构和铁含量变化可分为两代。早期形成的闪锌矿锌同位素组成(δ66Zn = 0.05‰~ 0.30‰)较晚形成的闪锌矿(δ66Zn = 0.30‰~ 0.60‰,Fe < 6 wt%)轻,铁含量(6 wt% ~ 10 wt%)较高,这可能是闪锌矿与成矿流体之间的瑞利型锌同位素分选所致。成矿流体来源于挥发物在累积模式下的大规模析出。铁锰碳酸盐矿物是主要的含锌脉石矿物,与晚期闪锌矿共生,δ66Zn值与晚期闪锌矿相似(0.24‰~ 0.41‰)。初始成矿流体的δ66Zn值估计在0.26‰左右,低于与矿相关和不相关的长英质岩δ66Zn值(0.23‰~ 0.69‰),进一步支持了流体析出作用在Zn同位素分馏中的作用。基于前期实验数据和理论模型,建立了含锌流体从长英质熔体释放到含锌成矿过程中新的锌同位素分馏模型。研究结果表明,热液流体中锌含量较长硅质残余熔体(即固化花岗岩)丰富,锌同位素组成较轻,锌同位素分选受岩浆-热液系统中释放流体和挥发性组分(Cl-和HS-)的影响。因此,锌同位素是追踪成矿过程的有力而灵敏的指标。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Zn isotopic variations in ore-related granite and ore minerals in a magmatic-hydrothermal deposit
Metal isotopes are powerful tools for investigating the migration and distribution of ore-forming elements. Zinc (Zn) is predominantly transported as chloride complexes in fluids, and its valence state remains relatively unaffected by redox conditions, thus Zn isotopes can provide valuable insights into the formation of magmatic-hydrothermal ore deposits. However, significant uncertainties persist regarding Zn isotopic fractionation in magmatic-hydrothermal systems during exsolution of hydrothermal fluids from silicic melts and crystallization of Zn-bearing minerals. The Lengshuikeng Ag–Pb–Zn deposit, one of the largest magmatic-hydrothermal Ag deposits in South China, was formed associated with the Mesozoic granitoid magmatism, and thus serves as an ideal natural laboratory for investigating Zn isotopic variations during the granite magmatism and hydrothermal mineralization. Systematic Zn isotope analyses were conducted on hydrothermal Zn-bearing ores, gangue minerals, and ore-related and unrelated felsic rocks. Sphalerite is the main ore mineral, which can be divided into two generations based on the “chalcopyrite disease” texture and Fe content variations. The early-formed sphalerite displays lighter Zn isotopic compositions (δ66Zn = 0.05 ‰ to 0.30 ‰) and higher Fe contents (6 wt% – 10 wt%) than the late-formed ones (δ66Zn = 0.30 ‰ to 0.60 ‰, Fe < 6 wt%), which probably resulted from Rayleigh-type Zn isotopic fractionation between sphalerite and ore-forming fluid. The ore-forming fluid was derived from large-scale exsolution of volatiles under a cumulative mode. Fe-Mn carbonate minerals are the main Zn-bearing gangue minerals, and they coexist with, and have similar δ66Zn values (0.24 ‰–0.41 ‰) to those of the late sphalerite. The estimated δ66Zn value of the initial ore-forming fluid is around 0.26 ‰, which is lower than those of the ore-related and unrelated felsic rocks (0.23 ‰–0.69 ‰), further supporting the role of fluid exsolution during the Zn isotopic fractionation. Based on the early experimental data and our theoretical modeling, a new Zn-isotope fractionation model has been reconstructed during the processes from Zn-bearing fluids released from the felsic melt to Zn-bearing mineralization. Our findings reveal that hydrothermal fluids are richer in Zn and have lighter Zn isotopic compositions than their felsic residual melts (i.e., solidified granites), and the Zn isotopic fractionation is influenced by amounts of the released fluids and volatile components (i.e., Cl- and HS-) in magmatic-hydrothermal systems. Therefore, Zn isotopes serve as powerful and sensitive indicators for tracing mineralization processes.
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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