首页> 外文期刊>Mineralium Deposita >Geothermal mineralized scales in the pipe system of the geothermal Piancastagnaio power plant (Mt. Amiata geothermal area): a key to understand the stibnite, cinnabarite and gold mineralization of Tuscany (central Italy)
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Geothermal mineralized scales in the pipe system of the geothermal Piancastagnaio power plant (Mt. Amiata geothermal area): a key to understand the stibnite, cinnabarite and gold mineralization of Tuscany (central Italy)

机译:Piancastagnaio地热发电厂(Amiata山地热区)的管道系统中的地热矿化垢:了解托斯卡纳(意大利中部)的辉锑矿,朱砂石和金矿化的关键

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The CO2-rich geothermal fluids produced in the Piancastagnaio geothermal field (Mt. Amiata geothermal area, Southern Tuscany, Italy) show temperatures up to 360°C and pressures of about 200 bar at depths of around 3,500 m (Giolito, Ph.D. thesis, Università degli Studi di Firenze, Italy, pp 1–147, 2005). CaCO3- and/or SiO2-dominated scales are deposited in the pipes leading to the pressure and atmospheric separators of the geothermal wells. High content of metastibnite and/or stibnite in both calcite and silica scales and Sb contents of up to 50 mg/L in the fluids indicate their mineralising potential. The red or black colours of the scales depend on the predominance of red metastibnite or black stibnite, respectively. In our condensation experiments, as well as during deposition of the scales, metastibnite is the first Sb2S3 mineral to form. In a second stage, metastibnite is transformed to stibnite. During depressurization the Hg content of geothermal fluids partitions preferentially into the gas phase, whereas Sb and As remain in the liquid phase. This separation explains the often observed areal separation of Hg and Sb mineralization. The multistage deposition of Sb in the mining district of Tuscany is due to a periodic restoration of the permeability of the ore-bearing faults by microseismic events and subsequent host rock brecciation. The still ongoing microseismic events are induced by the accumulation of high-pressure CO2-rich fluids along faults followed by mechanical failure of the faults.
机译:在Piancastagnaio地热田(意大利托斯卡纳南部的Amiata地热区)中产生的富含CO 2 的地热流体在3,500深度处显示出高达360°C的温度和约200 bar的压力m(Giolito,博士学位论文,意大利佛罗伦萨大学研究中心,第1至147页,2005年)。 CaCO 3 -和/或SiO 2 为主的水垢沉积在通往地热井的压力和大气分离器的管道中。方解石和二氧化硅垢中的变辉石和/或辉石的含量很高,并且流体中的Sb含量高达50 mg / L,表明它们具有矿化潜力。鳞片的红色或黑色分别取决于红色变辉石或黑色辉石的优势。在我们的凝结实验以及水垢沉积过程中,变质石是第一个形成的Sb 2 S 3 矿物。在第二阶段中,变辉石转变为辉石。在减压过程中,地热流体中的Hg含量优先分配到气相中,而Sb和As保留在液相中。这种分离解释了经常观察到的Hg和Sb矿化的区域分离。托斯卡纳矿区Sb的多阶段沉积是由于微地震事件和随后的主岩溶化作用使含矿断层的渗透性周期性恢复所致。沿断层的富CO 2 高压流体的聚集,继而引起断层的机械破坏,引起了仍在继续的微地震事件。

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