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From mantle to critical zone:A review of large and giant sized deposits of the rare earth elements

机译:从地幔到临界区:稀土元素的大型和巨型矿床回顾

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The rare earth elements are unusual when defining giant-sized ore deposits, as resources are often quoted as total rare earth oxide, but the importance of a deposit may be related to the grade for indi-vidual, or a limited group of the elements. Taking the total REE resource, only one currently known deposit (Bayan Obo) would class as giant (>1.7 ? 107 tonnes contained metal), but a range of others classify as large (>1.7 ? 106 tonnes). With the exception of unclassified resource estimates from the Olympic Dam IOCG deposit, all of these deposits are related to alkaline igneous activity e either car-bonatites or agpaitic nepheline syenites. The total resource in these deposits must relate to the scale of the primary igneous source, but the grade is a complex function of igneous source, magmatic crystal-lisation, hydrothermal modification and supergene enrichment during weathering. Isotopic data suggest that the sources conducive to the formation of large REE deposits are developed in subcontinental lithospheric mantle, enriched in trace elements either by plume activity, or by previous subduction. The reactivation of such enriched mantle domains in relatively restricted geographical areas may have played a role in the formation of some of the largest deposits (e.g. Bayan Obo). Hydrothermal activity involving fluids from magmatic to meteoric sources may result in the redistribution of the REE and increases in grade, depending on primary mineralogy and the availability of ligands. Weathering and supergene enrichment of carbonatite has played a role in the formation of the highest grade deposits at Mount Weld (Australia) and Tomtor (Russia). For the individual REE with the current highest economic value (Nd and the HREE), the boundaries for the large and giant size classes are two orders of magnitude lower, and deposits enriched in these metals (agpaitic systems, ion absorption deposits) may have significant economic impact in the near future.
机译:在定义巨型矿床时,稀土元素是不寻常的,因为资源通常被称为全部稀土氧化物,但是矿床的重要性可能与单个或少数元素的品位有关。以REE资源总量计,只有一个目前已知的矿床(Bayan Obo)可归类为巨型矿床(含金属> 1.7至107吨),但其他矿床则归类为大型(> 1.7至106吨)。除了奥林匹克大坝IOCG矿床的未分类资源估计以外,所有这些矿床都与碳酸盐岩或正长岩霞石正长岩的碱性火成岩活动有关。这些矿床中的总资源必须与主要火成岩源的规模有关,但品位是火成岩源,岩浆结晶,水热变质和风化过程中超基因富集的复杂函数。同位素数据表明,有利于形成大型REE矿床的来源是在陆下岩石圈地幔中发育的,通过羽流活动或先前的俯冲作用富集了微量元素。在相对有限的地理区域重新激活这些富集的地幔区域,可能在某些最大的矿床(例如,巴彦鄂博)的形成中发挥了作用。涉及岩浆到陨石流体的水热活动可能导致稀土元素的重新分布并增加品位,这取决于主要的矿物学和配体的可用性。碳酸盐岩的风化作用和超基因富集在Mount Weld(澳大利亚)和Tomtor(俄罗斯)的最高品位矿床形成中发挥了作用。对于当前经济价值最高的单个稀土元素(Nd和HREE),大尺寸和巨型尺寸类别的边界要低两个数量级,富含这些金属的沉积物(胶凝体系,离子吸收沉积物)可能具有显着的在不久的将来会对经济产生影响。

著录项

  • 来源
    《地学前缘(英文版)》 |2016年第3期|315-334|共20页
  • 作者单位

    School of Environment and Technology, University of Brighton, Lewes Road, Brighton BN2 4GJ, UK;

    Camborne School of Mines, University of Exeter, UK;

    Camborne School of Mines, University of Exeter, UK;

    Department of Earth and Environmental Sciences, University of St Andrews, UK d Department of Geology and Pedology, Mendel University, Brno, Czech Republic;

    Camborne School of Mines, University of Exeter, UK;

  • 收录信息 中国科学引文数据库(CSCD);中国科技论文与引文数据库(CSTPCD);
  • 原文格式 PDF
  • 正文语种 eng
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