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地球上“缺失”的铌可能存在于地核中。

The Earth's 'missing' niobium may be in the core.

作者信息

Wade J, Wood B J

机构信息

Department of Earth Sciences, University of Bristol, UK.

出版信息

Nature. 2001 Jan 4;409(6816):75-8. doi: 10.1038/35051064.

Abstract

As the Earth's metallic core segregated from the silicate mantle, some of the moderately siderophile ('iron-loving') elements such as vanadium and chromium are thought to have entered the metal phase, thus causing the observed depletions of these elements in the silicate part of the Earth. In contrast, refractory 'lithophile' elements such as calcium, scandium and the rare-earth elements are known to be present in the same proportions in the silicate portion of the Earth as in the chondritic meteorites-thought to represent primitive planetary material. Hence these lithophile elements apparently did not enter the core. Niobium has always been considered to be lithophile and refractory yet it has been observed to be depleted relative to other elements of the same type in the crust and upper mantle. This observation has been used to infer the existence of hidden niobium-rich reservoirs in the Earth's deep mantle. Here we show, however, that niobium and vanadium partition in virtually identical fashion between liquid metal and liquid silicate at high pressure. Thus, if a significant fraction of the Earth's vanadium entered the core (as is thought), then so has a similar fraction of its niobium, and no hidden reservoir need be sought in the Earth's deep mantle.

摘要

当地球的金属核心与硅酸盐地幔分离时,一些中等亲铁元素(即“爱铁”元素),如钒和铬,被认为进入了金属相,从而导致在地球的硅酸盐部分中观察到这些元素的贫化。相比之下,难熔亲石元素,如钙、钪和稀土元素,在地球的硅酸盐部分中的比例与球粒陨石(被认为代表原始行星物质)中的比例相同。因此,这些亲石元素显然没有进入地核。铌一直被认为是亲石且难熔的元素,但据观察,相对于地壳和上地幔中其他同类元素,铌出现了贫化。这一观察结果被用于推断地球深部地幔中存在隐藏的富铌储库。然而,我们在此表明,在高压下,铌和钒在液态金属和液态硅酸盐之间的分配方式几乎相同。因此,如果地球上很大一部分钒进入了地核(正如人们所认为的那样),那么类似比例的铌也进入了地核,无需在地球深部地幔中寻找隐藏的储库。

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