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Chemical and isotopic kinship of iron in the Earth and Moon deduced from the lunar Mg-Suite

机译:在地球和月亮中的铁的化学和同位素血缘关系从月球架套房推导出来

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摘要

The Moon and the Earth's mantle share many chemical and isotopic traits, leading to the prevailing theory that they were formed from similar material. Iron is one element that shows apparent differences between the two bodies, with models for the composition of the Moon having approximate to 1.5 times more FeO (12-14 wt.%), relative to the Earth's mantle (8 wt.%). This difference is mirrored in their isotope compositions, where lunar mare basalts have delta Fe-57 (per mille deviation of the Fe-57/Fe-54 ratio from the IRMM-014 standard) 0.1-0.2 parts per thousand higher than peridotitic rocks representative of Earth's mantle, a feature initially attributed to loss of isotopically light Fe following a giant impact. However, whether basaltic rocks are suitable analogues for the Moon's composition is debatable in the light of their distinct source regions that reflect the extensive lithological stratification of the lunar mantle. Here, we evaluate the iron isotope composition of the bulk Moon through the study of igneous cumulate rocks of the lunar highlands Magnesium Suite (Mg Suite). The delta Fe-57 of Mg Suite rocks spans a limited range, from 0.05 parts per thousand to 0.10 parts per thousand, with an average (+0.07 0.02 parts per thousand) that overlaps with Earth's mantle (+0.05 +/- 0.01 parts per thousand). similarities that extend to their Mg#s, where both reach 0.9. Numerical modelling of iron isotope fractionation during lunar magma ocean crystallisation shows that the Mg Suite should accurately reflect the composition of the bulk Moon, which is therefore +0.07 +/- 0.02 parts per thousand, indistinguishable from Earth's mantle but heavier than chondrites (-0.01 +/- 0.01 parts per thousand). Iron thus behaves coherently with other elements that condense at temperatures higher than Li in showing no isotopic difference between the Earth and Moon, suggesting element depletion on the Moon affected only the more volatile elements. Therefore, there is no cosmochemical basis for iron enrichment or depletion in the bulk Moon relative to the Earth's mantle, whose composition is an analogue for that of the Moon. (C) 2017 Elsevier B.V. All rights reserved.
机译:月亮和地球的地幔分享了许多化学和同位素的特质,导致它们由类似材料形成的普遍理论。铁是一个元素,其在两个体之间显示出明显差异,其中与地球的地幔(8重量%)相近的月亮的组成的模型具有近似的1.5倍(12-14重量%)。这种差异在其同位素组合物中镜像,其中月球母马沼气具有Delta Fe-57(来自IRMM-014标准的FE-57 / FE-54比率的PER-57 / FE-54比率)0.1-0.2份千分比高于Peridotitic岩石代表地球的地幔,一个特征最初归因于巨大的影响之后的同位素轻微的FE。然而,玄武岩岩石是否是月亮组合物的合适的类似物是借助于它们在其不同的源区的光临,反映了月球地幔的广泛岩性分层。在这里,我们通过研究月亮高地镁套房(MG套件)的Igneous Cullulate岩石的研究评估散装的铁同位素组成。 Mg套件岩石的Delta Fe-57跨越一个有限的范围,从0.05份千分之一到0.10份,平均(+0.07 0.02份)与地球的地幔重叠(+0.05 +/- 0.01零件千)。延伸到其MG#S的相似之处,其中达到0.9。月球岩浆海洋晶体中铁同位素分馏的数值模拟表明,MG套件应该准确反映散装月亮的组成,因此+0.07 +/- 0.02份千分之一,与地球的地幔难以区分,但比Chondrites重得更重(-0.01 +/- 0.01份千分之一)。因此,铁与其他元素相干,在高于李的温度下凝结在地球和月亮之间没有同位素差异,表明月球上的元素耗尽影响了更多的挥发性元素。因此,在散装的肉体相对于地球的地幔中没有含有钢铁富集或耗尽的辅助依据,其组成是月球的模拟。 (c)2017年Elsevier B.V.保留所有权利。

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