Rhenium residency in molybdenite, compressional textures and relationship to polytypism

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Geochimica et Cosmochimica Acta Pub Date : 2024-12-13 DOI:10.1016/j.gca.2024.12.012
Mao Tan, Yiping Yang, Xiao-Wen Huang, Jiaxin Xi, Nuo Li, Yu-Miao Meng, Liang Qi
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Abstract

Molybdenite has been established as a robust mineral for Re-Os isotope dating. However, higher-precision Re-Os molybdenite dating is necessary to accurately determine the absolute timing of metal mineralization and duration of ore-forming hydrothermal systems. To improve the precision and accuracy of molybdenite Re-Os dating, molybdenite from the Longmendian deposit—with its old age, heterogeneous distribution of Re, compression deformation, and complex polytypes—serves as a reference for enhancing the precision of in-situ Re-Os dating or grain-scale sampling during solution Re-Os isotope dating of molybdenite. High-resolution scanning transmission electron microscopy (TEM) analysis demonstrates that Re, Os, Pb, Bi, Cu, and Fe are incorporated into the molybdenite crystal through isomorphic substitution for Mo. Electron probe analysis shows that a single molybdenite grain exhibits heterogeneous textures consisting of Re-rich (∼0.29–0.82 wt%) and Re-poor (<0.29 wt%) domains. Some molybdenite grains have undergone compression deformation. Rhenium can be enriched in either the deformed or the undeformed domains of molybdenite grains. Compression deformation in some grains induces delamination cracks in Re-rich domains, facilitating ore-forming fluid infiltration and leading to an inhomogeneous distribution of Re and other elements in molybdenite grains. Re-rich domain in molybdenite is enriched in other metals, including Fe, Co, Zn, Pb, and Bi, due to the overprint of the hydrothermal fluids with a lower temperature and a relatively high oxygen fugacity, leading to the formation of heterogeneous molybdenite. Micro-X-ray diffraction (μXRD) and TEM analyses have revealed that both the Re-rich and Re-poor domains belong to the 2H1 polytype, indicating that Re concentration and distribution are not directly related to the polytype of molybdenite. The Re-poor and deformed domain of molybdenite shows the coexistence of 2H1 and 3R polytypes (in a ratio of 9:1), suggesting that compression deformation led to polytype transformation. Therefore, the diverse characteristics of molybdenite in the Longmendian deposit present challenges for obtaining primary Re-Os age information. Nondestructive pre-characterization of molybdenite is essential before dating to ensure age homogeneity. Molybdenite samples with an undeformed and uniform distribution of elements (Re) within molybdenite grains are suitable candidates for analysis. Our findings collectively offer strategies to enhance precision while advancing the understanding of elemental and isotopic geochemical behavior in the contexts of metamorphism, deformation, and fluid flow environments.
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辉钼矿已被确定为 Re-Os 同位素测年的可靠矿物。然而,要准确确定金属成矿的绝对时间和成矿热液系统的持续时间,就需要更高精度的辉钼矿Re-Os年代测定。为了提高辉钼矿Re-Os定年的精度和准确性,龙门甸矿床的辉钼矿--其年代久远、Re分布不均、压缩变形和复杂的多型性--可作为提高辉钼矿原位Re-Os定年或溶液Re-Os同位素定年过程中晶粒尺度取样精度的参考。高分辨率扫描透射电子显微镜(TEM)分析表明,Re、Os、Pb、Bi、Cu 和 Fe 是通过同构取代 Mo 的方式融入辉钼矿晶体的。电子探针分析表明,单个辉钼矿晶粒呈现出由富Re(0.29-0.82 wt%)和贫Re(0.29 wt%)域组成的异质纹理。一些辉钼矿晶粒经历了压缩变形。铼可在辉钼矿晶粒的变形或未变形域中富集。某些晶粒的压缩变形会在富铼域诱发分层裂纹,促进成矿流体的渗入,导致钼矿晶粒中的铼和其他元素分布不均。由于热液温度较低,氧富集度相对较高,导致形成异质辉钼矿,因此辉钼矿中的富集域富含其他金属,包括铁、钴、锌、铅和铋。显微 X 射线衍射(μXRD)和 TEM 分析表明,富 Re 域和贫 Re 域都属于 2H1 多晶型,表明 Re 的浓度和分布与辉钼矿的多晶型没有直接关系。辉钼矿的再贫域和变形域显示出 2H1 和 3R 多型共存(比例为 9:1),表明压缩变形导致了多型转化。因此,龙门甸矿床中辉钼矿的多样化特征为获取原始Re-Os年龄信息带来了挑战。在测年之前,必须对辉钼矿进行非破坏性预表征,以确保年龄的均一性。辉钼矿样品中的元素(Re)在辉钼矿晶粒内未变形且分布均匀,适合进行分析。我们的研究结果共同为提高精确度提供了策略,同时也推进了对变质、变形和流体流动环境下元素和同位素地球化学行为的理解。
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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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