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Implications for behavior of volatile elements during impacts—Zinc and copper systematics in sediments from the Ries impact structure and central European tektites

机译:对撞击过程中挥发性元素的行为的影响-里斯撞击结构和中欧陨石中沉积物中的锌和铜系统

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摘要

Moldavites are tektites genetically related to the Ries impact structure, located in Central Europe, but the source materials and the processes related to the chemical fractionation of moldavites are not fully constrained. To further understand moldavite genesis, the Cu and Zn abundances and isotope compositions were measured in a suite of tektites from four different substrewn fields (South Bohemia, Moravia, Cheb Basin, Lusatia) and chemically diverse sediments from the surroundings of the Ries impact structure. Moldavites are slightly depleted in Zn (~10–20%) and distinctly depleted in Cu (>90%) relative to supposed sedimentary precursors. Moreover, the moldavites show a wide range in δZn values between 1.7 and 3.7‰ (relative to JMC 3-0749 Lyon) and δCu values between 1.6 and 12.5‰ (relative to NIST SRM 976) and are thus enriched in heavy isotopes relative to their possible parent sedimentary sources (δZn = −0.07 to +0.64‰; δCu = −0.4 to +0.7‰). In particular, the Cheb Basin moldavites show some of the highest δCu values (up to 12.5‰) ever observed in natural samples. The relative magnitude of isotope fractionation for Cu and Zn seen here is opposite to oxygen-poor environments such as the Moon where Zn is significantly more isotopically fractionated than Cu. One possibility is that monovalent Cu diffuses faster than divalent Zn in the reduced melt and diffusion will not affect the extent of Zn isotope fractionation. These observations imply that the capability of forming a redox environment may aid in volatilizing some elements, accompanied by isotope fractionation, during the impact process. The greater extent of elemental depletion, coupled with isotope fractionation of more refractory Cu relative to Zn, may also hinge on the presence of carbonyl species of transition metals and electromagnetic charge, which could exist in the impact-induced high-velocity jet of vapor and melts.
机译:摩尔达伏特是与位于中欧的Ries撞击结构遗传相关的陨石,但是与摩尔达伏特的化学分馏有关的原材料和过程并未受到完全限制。为了进一步了解霉菌的成因,在来自四个不同次生田(南波希米亚,摩拉维亚,Cheb盆地,卢萨西亚)的一组陨石中以及来自Ries撞击结构周围的化学变化沉积物中测量了铜和锌的丰度和同位素组成。相对于假定的沉积前驱体,摩尔达维特的锌含量略低(约10-20%),而铜的含量则明显不足(> 90%)。此外,摩尔达分子显示的δZn值在1.7至3.7‰(相对于JMC 3-0749里昂)和δCu值在1.6至12.5‰(相对于NIST SRM 976)之间较宽,因此相对于它们而言富含重同位素。可能的母体沉积源(δZn= -0.07至+ 0.64‰;δCu= -0.4至+ 0.7‰)。特别是,Cheb盆地的霉菌显示出一些在自然样品中观察到的最高δCu值(高达12.5‰)。此处所见的Cu和Zn同位素分馏的相对幅度与氧气贫乏的环境(例如,月亮)相反,在月球中,Zn的同位素分馏率明显高于Cu。一种可能性是在还原的熔体中一价铜的扩散速度快于二价锌,扩散不会影响锌同位素分馏的程度。这些观察结果暗示形成氧化还原环境的能力可能有助于在撞击过程中挥发某些元素,并伴随同位素分级。元素耗竭程度的提高,再加上难熔的铜相对于锌的同位素分馏,也可能取决于过渡金属的羰基物质和电磁电荷的存在,这可能存在于撞击产生的蒸气和蒸汽的高速射流中。融化。

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