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A diffusion mechanism for core-mantle interaction

机译:地幔相互作用的扩散机制

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Understanding the geochemical behaviour of the siderophile elements — those tending to form alloys with iron in natural environments — is important in the search for a deep-mantle chemical 'fingerprint' in upper mantle rocks, and also in the evaluation of models of large-scale differentiation of the Earth and terrestrial planets. These elements are highly concentrated in the core relative to the silicate mantle, but their concentrations in upper mantle rocks are higher than predicted by most core-formation models. It has been suggested that mixing of outer-core material back into the mantle following core formation may be responsible for the siderophile element ratios observed in upper mantle rocks. Such re-mixing has been attributed to an unspecified metal-silicate interaction in the reactive D" layer just above the core-mantle boundary. The siderophile elements are excellent candidates as indicators of an outer-core contribution to the mantle, but the nature and existence of possible core-mantle interactions is controversial. In light of the recent findings that grain-boundary diffusion of oxygen through a dry intergranular medium may be effective over geologically significant length scales and that grain boundaries can be primary storage sites for incompatible lithophile elements, the question arises as to whether siderophile elements might exhibit similar (or greater) grain-boundary mobility. Here we report experimental results from a study of grain-boundary diffusion of siderophile elements through polycrystalline MgO that were obtained by quantifying the extent of alloy formation between initially pure metals separated by~l mm of polycrystalline MgO. Grain-boundary diffusion resulted in significant alloying of sink and source particles, enabling calculation of grain-boundary fluxes. Our computed diffu-sivities were high enough to allow transport of a number of siderophile elements over geologically significant length scales (tens of kilometres) over the age of the Earth. This finding establishes grain-boundary diffusion as a potential fast pathway for chemical communication between the core and mantle.
机译:了解亲铁元素的地球化学行为(那些在自然环境中倾向于与铁形成合金的元素)对于在上地幔岩石中寻找深地幔化学“指纹”以及评估大型模型具有重要意义。地球和地球行星的分化。这些元素相对于硅酸盐地幔高度集中在岩心中,但它们在上地幔岩石中的浓度高于大多数岩心形成模型所预测的浓度。已经提出,在岩心形成之后将外核材料混合回到地幔中可能是上地幔岩石中观察到的嗜铁元素比例的原因。这种重新混合归因于在核心-地幔边界上方的反应性D''层中未指定的金属-硅酸盐相互作用。嗜铁铁元素是极好的候选指标,可指示外核对地幔的贡献,但其性质和鉴于最近的发现,氧气在干燥的粒间介质中的晶界扩散可能在地质上很长的尺度上是有效的,并且晶界可能是不相容的亲石物质的主要储存位点,问题是嗜铁亲铁元素是否可能表现出相似(或更大)的晶界迁移率。在这里,我们报告了一项实验结果,该研究是通过量化多晶镁合金之间合金形成程度而获得的嗜铁亲铁元素通过多晶MgO的晶界扩散研究。最初的纯金属被约1毫米的多晶MgO隔开。导致沉颗粒和源颗粒的明显合金化,从而可以计算晶界通量。我们计算出的扩散系数足够高,可以在地球年龄范围内以地质学上显着的长度尺度(数十公里)运输大量嗜铁亲铁元素。这一发现将晶界扩散确定为核心与地幔之间化学通讯的潜在快速途径。

著录项

  • 来源
    《Nature》 |2007年第7170期|709-711|共3页
  • 作者单位

    Department of Earth and Environmental Sciences, Rensseiaer Polytechnic Institute, Troy, New York 12180, USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);美国《化学文摘》(CA);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 自然科学总论;
  • 关键词

  • 入库时间 2022-08-18 02:56:20

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