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DOI | 10.1016/j.epsl.2020.116468 |
Metal-silicate silicon isotopic fractionation and the composition of the bulk Earth | |
Moynier F.; Deng Z.; Lanteri A.; Martins R.; Chaussidon M.; Savage P.; Siebert J. | |
发表日期 | 2020 |
ISSN | 0012821X |
卷号 | 549 |
英文摘要 | The difference in the Si isotopic composition between the Earth and primitive meteorites had been used to constrain the amount of Si in the Earth's core. However, there is presently a debate on the magnitude of the isotopic fractionation between metal and silicates as function of temperature based on experimental data. Here, we use a natural sample, an enstatite meteorite, Itqyi, as a natural experiment to determine an independent Si isotopic fractionation factor between metal and silicate. We determined the temperature of equilibrium between metal and silicate as well as the Si isotopic composition between the phases. We find that the dependence of Si isotopes with temperature to be: [Formula presented] Using this dependence of the δ30Si with temperature we estimate the bulk Earth δ30Si as a function of Si content of the core for different plausible conditions. Even when using the most extreme parameters, we show that the bulk Earth must be isotopically heavier than any chondrites groups. We therefore confirm that core formation alone cannot account for the isotopic difference between the Earth and primitive meteorites. We show that there is no correlation between δ30Si and the Mg/Si ratio suggesting that forsterite fractionation in the solar nebula may have had only a limited effect, if any. Our new results therefore confirm that volatility should have had a fundamental effect in shaping terrestrial planets chemical composition. © 2020 Elsevier B.V. |
关键词 | accretioncore formationgeochemistryItqyimeteoritesplanetary differentiation |
英文关键词 | Geochemistry; Isotopes; Metals; Meteorites; Silicates; Chemical compositions; Isotopic composition; Isotopic fractionation factors; Isotopic fractionations; Metal silicates; Natural experiment; Primitive meteorites; Terrestrial planets; Silicon; chemical composition; core (planetary); isotopic fractionation; meteorite; silicate; silicon; trace metal |
语种 | 英语 |
来源期刊 | Earth and Planetary Science Letters |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/202800 |
作者单位 | Institut de Physique du Globe de Paris, Université de Paris, CNRS, 1 rue Jussieu, Paris, 75005, France; School of Earth and Environmental Sciences, University of St Andrews, Irvine Building, St Andrews, KY16 9AL, United Kingdom; Institut Universitaire de France, 103 boulevard Saint-Michel, Paris, 75005, France |
推荐引用方式 GB/T 7714 | Moynier F.,Deng Z.,Lanteri A.,et al. Metal-silicate silicon isotopic fractionation and the composition of the bulk Earth[J],2020,549. |
APA | Moynier F..,Deng Z..,Lanteri A..,Martins R..,Chaussidon M..,...&Siebert J..(2020).Metal-silicate silicon isotopic fractionation and the composition of the bulk Earth.Earth and Planetary Science Letters,549. |
MLA | Moynier F.,et al."Metal-silicate silicon isotopic fractionation and the composition of the bulk Earth".Earth and Planetary Science Letters 549(2020). |
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