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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Effect of silicon on activity coefficients of siderophile elements (Au, Pd, Pt, P, Ga, Cu, Zn, and Pb) in liquid Fe: Roles of core formation, late sulfide matte, and late veneer in shaping terrestrial mantle geochemistry
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Effect of silicon on activity coefficients of siderophile elements (Au, Pd, Pt, P, Ga, Cu, Zn, and Pb) in liquid Fe: Roles of core formation, late sulfide matte, and late veneer in shaping terrestrial mantle geochemistry

机译:硅Fe中硅Fe的磷酸化元素(Au,Pd,Pt,P,Ga,Cu,Zn和Pb)活性系数的影响:核心形成,晚硫化物遮罩和塑造地球化学地球化学中的晚期胶合的作用

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Earth's core contains similar to 10% of a light element that may be a combination of Si, S, C, O or H, with Si potentially being the major light element. Metal-silicate partitioning of siderophile elements can place important constraints on the P-T-fO(2) and composition of the early Earth, but the effect of Si alloyed in Fe liquids is unknown for many of these elements. In particular, the effect of Si on the partitioning of highly siderophile elements (Au, Re and PGE) is virtually unknown. To address this gap in understanding, we have undertaken a systematic study of the highly siderophile elements Au, Pd, and Pt, and the volatile siderophile elements P, Ga, Cu, Zn, and Pb at variable Si content of metal, and 1600 degrees C and 1 GPa. From our experiments we derive epsilon interaction parameters between these elements and Si in Fe metallic liquids. The new parameters are used to update an activity model for trace siderophile elements in Fe alloys; Si causes large variation in the magnitude of activity coefficients of these elements in FeSi liquids. Because the interaction parameters are all positive, Si causes a decrease in their metal/silicate partition coefficients. We combine these new activity results with experimental studies of Au, Pd, Pt, P, Ga, Cu, Zn and Pb, to derive predictive expressions for metal/silicate partition coefficients which can then be applied to Earth. The expressions are applied to two scenarios for continuous accretion of Earth; specifically for constant and increasing fO(2) during accretion. The results indicate that mantle concentrations of P, Ga, Cu, Zn, and Pb can be explained by metalsilicate equilibrium during accretion of the Earth where Earth's early magma ocean deepens to pressures of 40-60 GPa. Au, Pd, and Pt, on the other hand become too high in the mantle in such a scenario, and require a later removal mechanism, rather than an addition as traditionally argued. A late reduction event that removes 0.5% metal from a shallow magma
机译:地球的核心含有类似于光元件的10%,其可以是Si,S,C,O或H的组合,Si可能是主要的光元件。金属硅酸盐元素的硅酸盐分配可以对早期地球的P-T-FO(2)和组成来为早期地球的组成施加重要的约束,但是对于许多这些元素,Si合金化的Si的作用是未知的。特别地,Si对高度施手元件(Au,Re和PGE)的分区的影响几乎未知。为了解决理解的这种差距,我们已经对金属变量Si含量的高磷酸化元素Au,Pd和Pt和挥发性脱脂素元件P,Ga,Cu,Zn和Pb进行了系统研究,以及1600度C和1 GPA。从我们的实验来看,我们在Fe金属液体中衍生在这些元素和Si之间的epsilon相互作用参数。新参数用于更新Fe合金中的痕量三角形元素的活动模型; SI在FESI液体中导致这些元素的活动系数大小的大变化。因为相互作用参数均为正,Si导致其金属/硅酸盐分区系数的减少。我们将这些新的活性结果与Au,pd,pt,p,ga,Cu,Zn和Pb的实验研究结合起来,以推导出用于金属/硅酸盐分配系数的预测表达,然后可以将其施加到地球上。表达式应用于两种情况,用于连续增加地球;专门用于恒定和增加在增生期间的FO(2)。结果表明,P,Ga,Cu,Zn和Pb的搭腔浓度可以通过在地球的增生期间的金属硅酸盐均衡来解释,地球早期岩浆海洋深化40-60 GPa的压力。另一方面,在这种情况下,另一方面,在地幔中,稍后,并且需要稍后的去除机制,而不是传统上争论的加法。减少延迟事件,从浅岩浆中除去0.5%金属

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