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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Formation of hydrothermal tin deposits: Raman spectroscopic evidence for an important role of aqueous Sn(IV) species
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Formation of hydrothermal tin deposits: Raman spectroscopic evidence for an important role of aqueous Sn(IV) species

机译:水热锡沉积物的形成:拉曼光谱探测含水SN(IV)物种的重要作用

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摘要

The speciation of tin and the solubility of cassiterite in H2O + HCl were determined at temperatures to 600 degrees C using in situ Raman spectroscopy. In addition, information on the fluid-melt partition of Sn was obtained at 700 degrees C and indicated a preference of the fluid only at HCl concentrations that are much higher than in fluids exsolved from natural felsic melts. Dissolution of cassiterite generally resulted in formation of Sn(IV) species unless reduced conditions were generated by hydrogen permeation or carbohydrates in the starting material. The prevalent aqueous Sn(IV) species was [SnCl4(H2O)(2)](0), with additional [SnCl3(H2O)(3)](+) and [SnCl5(H2O)](-). The only detectable Sn(II) species was very likely [Sn(II)Cl-3](-). Cassiterite solubility increased with HCl concentration and was generally high in H2O+HCl fluids, with no strong dependencies on temperature, pressure, or the oxidation state of tin in the fluid. The Sn( IV) concentrations at 500 and 600 degrees C determined from the integrated v(1)[Sn(IV)-Cl] band intensity are in good agreement with literature data on the cassiterite solubility in H2O + HCl at oxygen fugacities along the hematite-magnetite buffer. The combined results from previous experimental studies and this study demonstrate that HCl molality is a crucial parameter for hydrothermal mobilization and transport of tin and for cassiterite precipitation, and that pH, pressure and temperature are less important. Current models on hydrothermal tin deposit formation need to be augmented to include Sn(IV)-Cl complexes as significant tin-transporting species. Irrespective of the oxidation state of tin in the fluid, cassiterite precipitates due to reaction of the hydrothermal fluid with the wall rock (greisen or skarn formation), dilution (mixing with meteoric water) or a decrease in the HCl activity in the aqueous liquid by boiling. A redox reaction is only required for tin transported as Sn( II) to be converted to Sn(IV). (C) 2017 Els
机译:使用原位拉曼光谱法在温度至600℃下测定H 2 O + HCl中的锡的形状和羰基钛矿的溶解度。另外,在700℃下获得有关Sn流体 - 熔体分配的信息,并仅在高于自然肠溶熔体渗透的流体中的HCl浓度下的流体偏好。除非通过在原料中通过氢渗透或碳水化合物产生降低的条件,否则羰基钛的溶解通常形成Sn(IV)物种。普遍的Sn水溶液(IV)物质是[SnCl4(H 2 O)(2)](0),其中另外的[SnCl 3(H 2 O)(3)](+)和[SnCl5(H 2 O)]( - )。唯一可检测的Sn(II)物种非常可能是唯一的[sn(ii)cl-3]( - )。咔铝溶解度随H​​Cl浓度而增加,H 2 O + HCl流体通常高,在流体中的温度,压力或锡的氧化状态下没有强的依赖性。 500和600℃的Sn(IV)浓度从集成V(1)[Sn(IV)-Cl]带强度与关于沿着H2O + HCL中的Cassiterite溶解度的文献数据吻合良好赤铁矿 - 磁铁矿缓冲液。来自先前实验研究的组合结果和本研究表明,HCl摩尔族溶液是用于水热动力和锡的传输和用于羰基沉淀的关键参数,并且pH,压力和温度不太重要。水热锡沉积物形成的目前的模型需要增加,包括Sn(IV)-Cl复合物作为显着的锡旋转物种。与流体中的锡的氧化状态无关,Cassiterite由于水热流体与壁岩(GREISEN或SKARN地层)的反应而沉淀,稀释(与MEERICIC水解)的稀释(混合)或水性液体中的HCl活性降低沸腾。仅作为Sn(II)转化为SN(IV)的Sn(II)所需的氧化还原反应。 (c)2017年ELS

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