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182 万年前有早期地幔分化产物长期保存的证据。

182W evidence for long-term preservation of early mantle differentiation products.

机构信息

Department of Geology, University of Maryland, College Park, MD 20742, USA.

出版信息

Science. 2012 Mar 2;335(6072):1065-9. doi: 10.1126/science.1216351. Epub 2012 Feb 16.

Abstract

Late accretion, early mantle differentiation, and core-mantle interaction are processes that could have created subtle (182)W isotopic heterogeneities within Earth's mantle. Tungsten isotopic data for Kostomuksha komatiites dated at 2.8 billion years ago show a well-resolved (182)W excess relative to modern terrestrial samples, whereas data for Komati komatiites dated at 3.5 billion years ago show no such excess. Combined (182)W, (186,187)Os, and (142,143)Nd isotopic data indicate that the mantle source of the Kostomuksha komatiites included material from a primordial reservoir that represents either a deep mantle region that underwent metal-silicate equilibration or a product of large-scale magmatic differentiation of the mantle. The preservation, until at least 2.8 billion years ago, of this reservoir-which likely formed within the first 30 million years of solar system history-indicates that the mantle may have never been well mixed.

摘要

晚期增生、早期地幔分异和核幔相互作用是可能在地球地幔中产生细微的(182)W 同位素非均一性的过程。28 亿年前的科斯托穆克莎科马提岩的钨同位素数据显示出相对于现代地球样品有明显的(182)W 过剩,而 35 亿年前的科马提岩的钨同位素数据则没有显示出这种过剩。(182)W、(186,187)Os 和(142,143)Nd 同位素综合数据表明,科斯托穆克莎科马提岩的地幔源区包括来自原始储层的物质,这可能代表经历了金属-硅酸盐平衡的深部地幔区域,或是地幔大规模岩浆分异的产物。该储层的保存时间至少到 28 亿年前,它很可能是在太阳系历史的头 3000 万年中形成的,这表明地幔可能从未很好地混合过。

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