Spatial and Metallogenic Relationships between Different Hydrothermal Vein Systems in the Southern Arburèse District (SW Sardinia).

Matteo L. Deidda, D. Fancello, Moroni Marilena, S. Naitza, Ignazio Scano
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Abstract

: The SW Sardinian basement hosts various ore deposits linked to geological processes active from Cambrian to post-Variscan times. In particular, the Southern Arburèse district hosts several granite-related W-Sn-Mo deposits and a 10 km-long system of Ni-Co-As-Bi-Ag ± Au bearing five-element veins. New investigations into the eastern and central parts of the district (Pira Inferida mine sector) were performed to understand the poorly documented spatial and metallogenic relationships between these systems. The granite-related deposits consist of massive wolframite-quartz (W-Bi-Te-Au) and molybdenite-quartz veins, linked to the early Permian (289 ± 1 Ma) Mt. Linas granite, that are cross-cut by the five-element veins. The wolframite-quartz veins, observed by optical and electron (SEM-EDS) microscopy, show abundant native Bi, Bi-Te phases and native Au suggesting a W-Bi-Te-Au hydrothermal system. The five-element veins exhibit breccia and cockade textures, enveloping clasts of the Ordovician host-rocks and locally small fragments of the earlier W-Mo-quartz veins. The five-element vein paragenesis includes three main stages, from older to younger: (1) native elements (Bi ± Au); (2) Ni-Co arsenides-sulfarsenides in quartz gangue; and (3) Pb-Zn-Cu ± Ag sulfides in siderite gangue. The mineralogical, geochemical and isotopic features of the five-element vein swarm are closely comparable to five-element deposits elsewhere in Europe (Germany, Switzerland, Italian Alps). While the source of Ni and Co is still unknown, the high Bi contents, as well as Au enrichment in the five-element veins, suggest selective remobilization of these elements, and perhaps others, from the granite-related W-Bi-Te-Au veins. The five-element vein system was likely formed during a post-289 ± 1 Ma and post-Variscan metallogenic event.
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撒丁岛南部arbur区不同热液脉系空间成矿关系
撒丁岛西南基底拥有各种矿床,这些矿床与寒武纪至后瓦里斯坎时代活跃的地质过程有关。特别是南arbur地区赋存多处与花岗岩有关的W-Sn-Mo矿床和长10 km的含Ni-Co-As-Bi-Ag±Au的五元素脉体体系。对该区东部和中部地区(Pira interida矿区)进行了新的调查,以了解这些系统之间记录不足的空间和成矿关系。与花岗岩有关的矿床由块状黑钨矿石英(W-Bi-Te-Au)和辉钼矿石英脉组成,与早二叠世(289±1 Ma) Linas山花岗岩相连,由五元素脉交叉切割而成。通过扫描电镜和电子能谱(SEM-EDS)观察,黑钨矿-石英矿脉显示出丰富的原生Bi、Bi- te相和原生Au,表明存在W-Bi-Te-Au热液体系。五元素脉呈角砾岩和帽带状,包裹着奥陶系寄主岩的碎屑,局部包裹着早期钨钼石英脉的小碎片。五行脉共生由老向新分为三个主要阶段:(1)原生元素(Bi±Au);(2)石英脉石中镍钴砷化物-硫化物;(3)菱铁矿脉石中Pb-Zn-Cu±Ag硫化物。五元素脉群的矿物学、地球化学和同位素特征与欧洲其他地区(德国、瑞士、意大利阿尔卑斯山)的五元素矿床非常相似。虽然镍和钴的来源尚不清楚,但高Bi含量和金在五元素脉中的富集表明,这些元素和其他元素可能来自花岗岩相关的W-Bi-Te-Au脉。五行脉系可能形成于后289±1 Ma和后variscan成矿事件。
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