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Ruthenium isotope vestige of Earth's prelate-veneer mantle preserved in Archaean rocks

机译:保存在古生岩石中的地球上层-中层地幔的钌同位素痕迹

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摘要

The accretion of volatile-rich material from the outer Solar System represents a crucial prerequisite for Earth to develop oceans and become a habitable planet(1-4). However, the timing of this accretion remains controversial(5-8). It has been proposed that volatile elements were added to Earth by the late accretion of a late veneer consisting of carbonaceous-chondrite-like material after core formation had ceased(6,9,10). This view could not be reconciled with the ruthenium (Ru) isotope composition of carbonaceous chondrites(5,11), which is distinct from that of the modern mantle(12), or of any known meteorite group(5). As a possible solution, Earth's pre-late-veneer mantle could already have contained a fraction of Ru that was not fully extracted by core formation(13). The presence of such pre-late-veneer Ru can only be established if its isotope composition is distinct from that of the modern mantle. Here we report the first high-precision, mass-independent Ru isotope compositions for Eoarchaean ultramafic rocks from southwest Greenland, which display a relative Ru-100 excess of 22 parts per million compared with the modern mantle value. This Ru-100 excess indicates that the source of the Eoarchaean rocks already contained a substantial fraction of Ru before the accretion of the late veneer. By 3.7 billion years ago, the mantle beneath southwest Greenland had not yet fully equilibrated with late accreted material. Otherwise, no Ru isotopic difference relative to the modern mantle would be observed. If constraints from other highly siderophile elements besides Ru are also considered(14), the composition of the modern mantle can only be reconciled if the late veneer contained substantial amounts of carbonaceous-chondrite-like materials with their characteristic Ru-100 deficits. These data therefore relax previous constraints on the late veneer and are consistent with volatile-rich material from the outer Solar System being delivered to Earth during late accretion.
机译:来自外部太阳系的富挥发性物质的积累是地球发展海洋并成为宜居星球的关键先决条件(1-4)。但是,这种增生的时间仍然存在争议(5-8)。有人提出,在岩心形成停止后,通过后期积聚由碳质球粒状材料组成的后期胶合板的后期积聚,将挥发性元素添加到地球上(6,9,10)。这种观点与碳质球粒陨石(5,11)的钌(Ru)同位素组成不符,这与现代地幔(12)或任何已知的陨石族(5)截然不同。作为一种可能的解决方案,地球上晚期的前地幔可能已经包含了一部分未被核心形成完全提取的Ru(13)。只有在其同位素组成与现代地幔的同位素组成不同的情况下,才能确定这种晚露头的Ru的存在。在这里,我们报道了格陵兰西南部的太古宙超镁铁质岩石的第一个高精度,与质量无关的Ru同位素组成,与现代地幔值相比,其Ru-100过量相对于百万分之22。 Ru-100的过量表明在晚胶合板积聚之前,Eoarchaean岩石的来源已经包含了大部分的Ru。到了37亿年前,格陵兰西南部的地幔还没有与后期积聚的物质完全平衡。否则,将不会观察到相对于现代地幔的Ru同位素差异。如果还考虑了除Ru以外的其他高度亲铁性元素的限制因素(14),则只有在后期胶合板包含大量具有Ru-100缺陷的碳质球粒状材料的情况下,才能协调现代地幔的组成。因此,这些数据放松了后期对单板的限制,并且与后期吸积过程中来自外部太阳系的富含挥发性物质的物质被传递到地球相一致。

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  • 来源
    《Nature》 |2020年第7798期|240-244|共5页
  • 作者单位

    Univ Cologne Inst Geol & Mineral Cologne Germany;

    Univ Copenhagen Dept Geosci & Nat Resource Management Copenhagen Denmark;

    Cardiff Univ Sch Earth & Ocean Sci Cardiff Wales;

    Kanazawa Univ Inst Sci & Engn Fac Geosci & Civil Engn Kanazawa Ishikawa Japan|Columbia Univ Lamont Doherty Earth Observ New York NY USA|Japan Agcy Marine Earth Sci & Technol Volcanoes & Earths Interior Res Ctr Res Inst Marine Geodynam Yokosuka Kanagawa Japan;

    Univ New South Wales Australian Ctr Astrobiol Sydney NSW Australia;

    Geol Survey Western Australia East Perth WA Australia;

  • 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
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  • 入库时间 2022-08-18 04:58:22

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