A review of W and Sn isotopes and insights into their emerging applications in ore deposit geology

地质学 同位素 地球化学 锡石 矿化(土壤科学) 同位素地球化学 同位素分馏 热液循环 稳定同位素比值 矿物学 化学 古生物学 土壤水分 土壤科学 物理 量子力学 有机化学
作者
Zhaoyang Luo,Huan Li,Majid Ghaderi,Dapeng Zhu,Weicheng Jiang,Jing‐Hua Wu
出处
期刊:International Geology Review [Taylor & Francis]
卷期号:67 (3): 381-404 被引量:4
标识
DOI:10.1080/00206814.2024.2392255
摘要

In recent years, the advancements in multi-collector inductively coupled plasma mass spectrometry (MC – ICP – MS) technology have significantly enhanced our understanding of the isotopic variations in tungsten (W) and tin (Sn) among natural samples. The application of W isotopic fractionation (δ186/184W NIST 3163) has emerged in tracing the material cycle associated with solid Earth evolution as an excellent indicator. Also, the findings of Sn isotopic fractionation (e.g. δ122/118Sn 3161a) in cassiterite have achieved initial success in revealing magmatic-hydrothermal processes. However, the mechanisms responsible for variations in W and Sn isotopes in the ore-forming processes remain to be fully addressed, and there is an urgent need to apply the W – Sn isotope systematics to geology (especially for ore deposit geology). In this contribution, the high-precision analytical methods for W and Sn isotopes, the significant variability in isotopic compositions, and the immense functionality of the tracing process are systematically summarized and reviewed. Conclusively, the prospects of the application of W and Sn isotopes in geology are listed, and it is pointed out that it is urgent to introduce W – Sn double isotope systematics into the study of ore deposits, apply the stable isotopic method for tracing the source of ore-forming materials and modelling the evolution of W and Sn isotopes in W – Sn metallogenic system. Focusing on the composition variations of W and Sn isotopes in magmatic-hydrothermal evolution is expected to explore the fractionation mechanism of those isotopes in the mineralization process from multiple perspectives, establishing the evolution model of W and Sn isotopes in the complex W – Sn metallogenic system, which can provide a fresh approach for in-depth understanding of the genesis of W – Sn mineralization, and then facilitating a new perspective for the study of large-scale W – Sn polymetallic mineralization.
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