埃及东南部沙漠Derhib硫化物-滑石矿床地质地球化学演化:矿床成因和交代蚀变的启示

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Mohamed Faisal , Huan Li , Rub'son N'nahano Heritier , Muhammad A. Gul , Farah A. Khedr , Zhekai Zhou , Sobhi M. Ghoneim
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引用次数: 0

摘要

滑石蚀变是各种矿床类型的特征,包括岩浆、热液和变质系统。在阿拉伯-努比亚盾(ANS)中,Shadli成矿带(埃及东南部沙漠)内的Derhib矿床是一个复杂的含金硫化物-滑石体系。尽管有历史上的采矿兴趣,但该矿床仍未使用先进的分析技术进行勘探,阻碍了我们对矿石沉淀的物理化学条件和机制的理解。采用了综合野外观测、岩石学调查和地球化学-同位素分析(全岩石地球化学、U-Pb-Lu-Hf年代学、锆石和硫化物化学以及S同位素)的综合方法。Derhib剪切带流纹岩熔岩呈钙碱性、铝质至过铝质组成,富Ba、Th、Nd、U、Zr和Sm,贫Nb、Ta、P和Sr,反映了与俯冲有关的岛弧岩浆作用。现场关系和地球化学特征表明,Derhib滑石矿床为碳酸盐岩原岩,证据如下:(a)白云岩附近存在绿泥石,(b) Cr、Ni和Co浓度低,(c) ΣREE与Zr、Hf和Th呈正相关,(d)滑石矿石与沉积样品的稀土模式相似,(e)滑石岩石的Y/Ho比与碳酸盐岩一致,(f)碳酸盐单元继承的稀土枯竭。(g)没有VMS变更区。高度剪切流纹岩熔岩的岩浆锆石年龄与Shadli变质火山(~ 695 Ma)基本一致,而再结晶锆石的锆石年龄为137.5±1.1 Ma,与埃及东部沙漠的上白垩世火山期一致。锆石微量元素、初始εHf(t)值(- 10.5 ~ - 17.8)和Hf地壳模式年龄(1.68 ~ 2.15 Ga)表明其成因与地壳作用密切相关。此外,硫化物、绿泥石和滑石的矿物化学特征以及硫化物δ34S值(−7.57‰~ +3.48‰)表明,与高度变形的富滑石岩石相关的硫化物具有表观成因特征,表明岩石通过原有硫化物矿石的再活化对硫的贡献。构造线是成矿流体的通道,在ANS地壳演化过程中为金属沉淀创造了有利的场所。该研究对形成Derhib硫化物-滑石矿床的地质和地球化学过程提供了有价值的见解。然而,需要进一步的地质年代学和同位素研究来充分了解共生序列和矿床成因。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Geological and geochemical evolution of the Derhib sulfide-talc deposit in the South Eastern Desert, Egypt: Insights into ore genesis and metasomatic alteration
Talc alteration is a characteristic feature of various ore deposit types, including magmatic, hydrothermal, and metamorphic systems. In the Arabian-Nubian Shield (ANS), the Derhib deposit within the Shadli Metallogenic Belt (South Eastern Desert, Egypt) represents a complex auriferous sulfide-talc system. Despite historical mining interest, the deposit remains underexplored using advanced analytical techniques, hindering our understanding of the physiochemical conditions and mechanisms governing ore precipitation. An integrated approach combining intensive field observations, petrographic investigations, and geochemical-isotopic analyses (whole rock geochemistry, U-Pb-Lu-Hf geochronology, zircon and sulfide chemistry, and S isotopes) was employed. Rhyolitic lavas in the Derhib shear zone exhibit calc-alkaline, metaluminous to peraluminous compositions, enriched in Ba, Th, Nd, U, Zr, and Sm but depleted in Nb, Ta, P, and Sr, reflecting subduction-related island-arc magmatism. Field relationships and geochemical signatures indicate a carbonate protolith for the Derhib talc deposit, evidenced by (a) the presence of chlorite adjacent to dolomite, (b) low Cr, Ni, and Co concentrations, (c) positive correlations between ΣREE and Zr, Hf, and Th, (d) similarities in REE patterns between talc ore and sedimentary samples, (e) a Y/Ho ratio in the talcose rocks aligns with carbonates rocks, (f) REE depletion inherited from carbonate units, and (g) the absence of VMS alteration zones. Magmatic zircon ages from highly sheared rhyolitic lava are largely consistent with the Shadli metavolcanics (∼695 Ma), while recrystallized zircons yield a concordia age of 137.5 ± 1.1 Ma, attributed to Upper Cretaceous volcanic episodes in the Egyptian Eastern Desert. Zircon trace elements, initial εHf(t) values (−10.5 to −17.8), and Hf crustal model ages (1.68 Ga to 2.15 Ga) indicate significant crustal involvement in their genesis. Additionally, the mineral chemistry of sulfide, chlorite, and talc, along with the sulfide δ34S values (−7.57 ‰ to +3.48 ‰), reveals that the sulfides associated with highly deformed talc-rich rocks display epigenetic features, suggesting sulfur contribution from country rocks through remobilization of pre-existing sulfide ores. Structural lineaments acted as channels for mineralizing fluids, creating favorable sites for metal precipitation during ANS crustal evolution. This study provides valuable insights into the geological and geochemical processes shaping the Derhib sulfide-talc deposit. However, further geochronological and isotopic investigations are needed to fully constrain paragenetic sequence and ore genesis.
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来源期刊
Lithos
Lithos 地学-地球化学与地球物理
CiteScore
6.80
自引率
11.40%
发文量
286
审稿时长
3.5 months
期刊介绍: Lithos publishes original research papers on the petrology, geochemistry and petrogenesis of igneous and metamorphic rocks. Papers on mineralogy/mineral physics related to petrology and petrogenetic problems are also welcomed.
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