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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >The effect of core composition on iron isotope fractionation between planetary cores and mantles
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The effect of core composition on iron isotope fractionation between planetary cores and mantles

机译:核心组合物对行星芯和幔型铁同位素分馏的影响

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We have conducted high-pressure, high-temperature isotope exchange experiments between molten silicate and molten Fe-Si-C-alloys to constrain the effect of Si on equilibrium Fe isotope fractionation during planetary core formation. The values of Delta Fe-57(Metal-Silicate) at 1850 degrees C and 1 GPa determined by high-resolution MC-ICP-MS in this study range from -0.013 +/- 0.054 parts per thousand (2SE) to 0.072 +/- 0.085 parts per thousand with 1.34-8.14 atom % Si in the alloy, respectively. These results, although not definitive on their own, are consistent with previous experimental results from our group and a model in which elements that substitute for Fe atoms in the alloy structure (i.e., Ni, S, and Si) induce a fractionation of Fe isotopes between molten silicate and molten Fe-alloys during planetary differentiation. Using in situ synchrotron X-ray diffraction data for molten Fe-rich alloys from the literature, we propose a model to explain this fractionation behavior in which impurity elements in Fe-alloys cause the nearest neighbor atomic distances to shorten, thereby stiffening metallic bonds and increasing the preference of the alloy for heavy Fe isotopes relative to the silicate melt. This fractionation results in the bulk silicate mantles of the smaller terrestrial planets and asteroids becoming isotopically light relative to chondrites, with an enrichment of heavy Fe isotopes in their cores, consistent with magmatic iron meteorite compositions. Our model predicts a bulk silicate mantle delta Fe-57 ranging from -0.01 parts per thousand to -0.12 parts per thousand for the Moon, -0.06 parts per thousand to -0.33 parts per thousand for Mars, and -0.08 parts per thousand to B -0.33 parts per thousand for Vesta. Independent estimates of the delta Fe-57 of primitive mantle source regions that account for Fe isotope fractionation during partial melting agree well with these ranges for all three planetary bodies and suggest that Mars and Vesta have cores wit
机译:我们在熔融硅酸盐和熔融Fe-Si-C合金之间进行了高压,高温同位素交换实验,以限制Si在行星芯形成过程中对平衡Fe同位素分馏的影响。在本研究中,通过高分辨率MC-ICP-MS测定的ΔFE-57(金属硅酸盐)的值在该研究范围内从-0.013 +/- 0.054份(2se)至0.072 + / - 合金中,0.085份每千份,含有1.34-8.14原子%Si。这些结果虽然不是本身的确定性,但是与我们的组和替代合金结构中的Fe原子的元素(即,Ni,S和Si)的模型的模型一致,其中诱导Fe同位素的分馏在行星分化期间熔融硅酸盐和熔融Fe-合金之间。使用原位同步X射线衍射数据从文献中熔融Fe-Richoly合金,我们提出了一种模型来解释该分馏行为,其中Fe-合金中的杂质元素导致最近的邻国原子距离缩短,从而加强金属粘合和增加合金相对于硅酸盐熔体的重氢同位素的优选。该分馏导致较小的地球行星的散装硅酸盐罩和小行星相对于白葡萄酒具有同位性光,其核心中的重型Fe同位素富集,与岩浆铁陨石组合物一致。我们的模型预测月亮的-0.01份000.01份000.0.0.12份批量硅酸盐硅酸盐ΔFe-57,为MAR的千分之一至-0.33份千分之一至-0.33份。 - 0.08零件至b -0.33 Vesta每千元。在部分熔点期间占Fe同位素分馏的原始地幔源区的独立估计与所有三个行星机构的这些范围都很好地同意,并表明火星和Vesta有机智

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