首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Nickel isotopic compositions of ferromanganese crusts and the constancy of deep ocean inputs and continental weathering effects over the Cenozoic
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Nickel isotopic compositions of ferromanganese crusts and the constancy of deep ocean inputs and continental weathering effects over the Cenozoic

机译:锰铁壳的镍同位素组成以及深海输入的恒定性和新生代的大陆风化作用

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The global variability in nickel (Ni) isotope compositions in ferromanganese crusts is investigated by analysing surface samples of 24 crusts from various ocean basins by MC-ICPMS, using a double-spike for mass bias correction. Ferromanganese crusts have δ60Ni isotopic compositions that are significantly heavier than any other samples thus far reported (-0.1‰ to 0.3‰), with surface scrapings ranging between 0.9‰ and 2.5‰ (relative to NIST SRM986). There is no well resolved difference between ocean basins, although the data indicate somewhat lighter values in the Atlantic than in the Pacific, nor is there any evidence that the variations are related to biological fractionation, presence of different water masses, or bottom water redox conditions. Preliminary data for laterite samples demonstrate that weathering is accompanied by isotopic fractionation of Ni, which should lead to rivers and seawater being isotopically heavy. This is consistent with the slightly heavier than average isotopic compositions recorded in crusts that are sampled close to continental regions. Furthermore, the isotopic compositions of crusts growing close to a hydrothermal source are clustered around ~1.5‰, suggesting that hydrothermal fluids entering the ocean may have a Ni isotopic composition similar to this value. Based on these data, the heavy Ni isotopic compositions of ferromanganese crusts are likely due to input of isotopically heavy Ni to the ocean from continental weathering and possibly also from hydrothermal fluids. A depth profile through one crust, CD29-2, from the north central Pacific Ocean displays large variations in Ni isotope composition (1.1-2.3‰) through the last 76Myr. Although there may have been some redistribution of Ni associated with phosphatisation, there is no systematic difference in Ni isotopic composition between deeper, older parts and shallower, younger parts of the crust, which may suggest that oceanic sources and sinks of Ni have largely remained in steady state over the Cenozoic. Additionally, the isotope profile is in agreement with a profile of Mn concentration through the same crust. This implies a link between the Ni isotopic composition recorded in ferromanganese crusts and the release of Ni into the ocean through hydrothermal activity. This supports the conclusions drawn from surface data, that Ni isotope ratios in ferromanganese crusts are largely controlled by the isotopic compositions of the Ni oceanic input sources.
机译:通过用MC-ICPMS分析来自两个海洋盆地的24个地壳的表面样本,并使用双尖峰进行质量偏差校正,研究了铁锰地壳中镍(Ni)同位素组成的全球变化。铁锰结壳的δ60Ni同位素组成比迄今报道的任何其他样品都重得多(-0.1‰至0.3‰),表面刮擦范围为0.9‰至2.5‰(相对于NIST SRM986)。尽管数据表明大西洋上的值比太平洋上的值稍轻,但各海盆之间没有很好解决的差异,也没有任何证据表明这种变化与生物分离,不同水团的存在或底水氧化还原条件有关。 。红土样品的初步数据表明,风化伴随着Ni的同位素分馏,这将导致河流和海水同位素变重。这与在靠近大陆地区采样的地壳中记录的同位素组成略高于平均同位素组成相符。此外,靠近热液源生长的地壳的同位素组成聚集在约1.5‰附近,这表明进入海洋的热液可能具有与该值相似的Ni同位素组成。基于这些数据,铁锰结壳的重Ni同位素组成很可能是由于大陆风化以及热液流体向海洋输入了同位素重Ni所致。从太平洋中北部穿过一个地壳CD29-2的深度剖面显示,直到最后76年来,Ni同位素组成(1.1-2.3‰)变化很大。尽管可能发生了与磷化有关的镍再分布,但地壳的深部,较老部分和较浅,较年轻的部分之间的镍同位素组成没有系统的差异,这可能表明镍的海洋来源和汇在很大程度上仍存在于地壳中。新生代处于稳态。另外,同位素分布与通过相同地壳的Mn浓度分布一致。这意味着铁锰结壳中记录的Ni同位素组成与通过水热活动将Ni释放到海洋中之间存在联系。这支持了从表面数据得出的结论,即锰铁壳中的Ni同位素比在很大程度上受Ni海洋输入源的同位素组成控制。

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