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首页> 外文期刊>Marine Geology >Uptake of elements from seawater by ferromanganese crusts: solid-phase associations and seawater speciation
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Uptake of elements from seawater by ferromanganese crusts: solid-phase associations and seawater speciation

机译:锰铁壳对海水中元素的吸收:固相缔合和海水形态

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摘要

Marine Fe-Mn oxyhydroxide crusts form by precipitation of dissolved components from seawater. Three hydrogenetic crust samples (one phosphatized) and two hydrothermal Mn-oxide samples were subjected to a sequential-leaching procedure in order to determine th host phases of 40 elements. Those host-phase associations are discussed with respect to element speciation in seawater. The partitioning of elements between the two major phases, Mn oxide and Fe oxyhydroxide, can in a first-order approximation be explained by a simple sorption model related to the inorganic speciation of the elements in seawater, as has been proposed in earlier models. Free and weakly complexed cations, such as alkali and alkaline earth metals, Mn, Co, Ni, Zn, Tl(I), and partly Y, are sorbed preferentially on the negatively charged surface of the MnO_2 in hydrogenetic crusts. The driving force is a strong coulombic interaction. All neutral or negatively charged chloro (Cd, Hg, Tl), carbonate (Cu, Y, Pb, and U), and hydroxide (Be, Sc, Ti, Fe, Zr, Nb, In, Sn, Sb, Te, Hf, Ta, Bi, Th, and Tl(III) complexes and oxyanions (V, Cr, As, Se, Mo, and W) bind to the slightly positively charged surface of the amorphous FeOOH phase. While coulombic interaction can explain the sorption of the negatively charged species, the binding of neutral species is based on specific chemical interaction. Organic complexation of elements in deep-ocean water seems to be at most of minor importance. Surface oxidation can explain some strong metal associations, e.g. of Co and Tl with the MnO_2 and Te with the FeOOH. Sorption reactions initially driven by coulombic forces are often followed by the formation of specific bonds between the adsorbate and the atoms of the oxide surface. Differences in the associations of some metals between the non-phosphatized and phosphatized hydrogenetic crusts and between the hydrogenetic and the hydrothermal samples reflect the different physico-chemical environments of formation and speciations in oxic seawater vs. less-oxic fluids, especially for the redox-sensitive metals such as Mo and V. These environmental-related differences indicate that the methodology of chemical speciation used here in combination with spectroscopic methods may allow for the detection of changes in paleoceanographic conditions recorded during the several tens of millions of years of crust growth.
机译:海水中的Fe-Mn羟基氢氧化物结皮是由溶解的成分沉淀而成。为了确定第40个元素的主体相,对三个氢化地壳样品(一个已磷酸盐化)和两个水热锰氧化物样品进行了连续浸出程序。讨论了那些宿主阶段的关联,涉及海水中的元素形态。 Mn氧化物和Fe OH氧化物这两个主要相之间的元素分配可以通过一阶近似来解释,该模型与海水中元素的无机形态有关,是一个简单的吸附模型,正如先前模型中所提出的那样。游离和弱络合的阳离子(例如碱金属和碱土金属,Mn,Co,Ni,Zn,Tl(I)和部分Y)优先吸附在氢脆皮中MnO_2的带负电荷的表面上。驱动力是强大的库仑相互作用。所有中性或带负电荷的氯(Cd,Hg,Tl),碳酸盐(Cu,Y,Pb和U)和氢氧化物(Be,Sc,Ti,Fe,Zr,Nb,In,Sn,Sb,Te,Hf ,Ta,Bi,Th和Tl(III)配合物和含氧阴离子(V,Cr,As,Se,Mo和W)结合到非晶态FeOOH相的带正电的表面上,而库仑相互作用可以解释对于带负电荷的物种,中性物种的结合是基于特定的化学相互作用,深海水中的元素有机络合似乎至多重要,表面氧化可以解释某些强金属缔合,例如Co和Tl与MnO_2和Te与FeOOH。最初由库仑力驱动的吸附反应通常是在被吸附物和氧化物表面原子之间形成特定的键,非磷酸化和磷酸化氢原子之间某些金属缔合的差异地壳,在水热与水热之间l样品反映了含氧海水与含氧量较低的液体(尤其是对钼和钒等氧化还原敏感金属)形成和形成的不同物理化学环境,这些与环境有关的差异表明此处使用的化学形成方法结合光谱方法可以检测到在几千万年的地壳生长过程中记录的古海洋学条件的变化。

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