The partitioning of selenium and tellurium between sulfide liquid and silicate melt and their abundances in the silicate Earth

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Zhiwei Liu , Yuan Li
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引用次数: 0

Abstract

Near-chondritic relative abundances of sulfur (S), selenium (Se), and tellurium (Te) observed in mantle peridotites have been used to support the hypothesis of a carbonaceous chondrite-like late veneer added to the proto-Earth. However, the extent to which the observed S, Se, and Te compositions represent the signature of the silicate Earth remains a topic of debate. The concentrations of Se and Te in mantle-derived melts, such as mid-ocean ridge basalts (MORBs), can help clarify this issue, provided we have a precise understanding of the behavior of Se and Te during magmatic differentiation and mantle partial melting. Here we conduct laboratory experiments to determine the sulfide liquid–silicate melt partition coefficients of Se and Te (DSe,TeSul/Sil) at crust–mantle conditions. Our results indicate that DSe,TeSul/Sil range from 180 to 2200 for Se and from 1000 to 25,400 for Te, exhibiting an inverted U-shaped dependence on the FeOtot content in silicate melt. We parameterize DSe,TeSul/Sil as a multi-function of the compositions of silicate melt and sulfide liquid, with pressure (0.5–2.5 GPa), temperature (1273–1973 K), and oxygen fugacity (FMQ-5 to FMQ+1.5; FMQ refers to the fayalite–magnetite–quartz buffer) having negligible effects on DSe,TeSul/Sil. Applying our parameterization to magmatic differentiation can effectively account for the Se, Te, and Cu systematics observed in both MORBs and oxidized arc magmas. More significantly, when applied to mantle partial melting, alongside high-precision Se and Te concentration data from MORBs, our parameterization yields superchondritic S/Se, S/Te, and Se/Te ratios in the depleted MORB mantle and primitive mantle, compared to carbonaceous chondrites. These findings suggest that the S, Se, and Te abundances in the silicate Earth were likely established during the main accretion phase, with the late veneer playing only a minor role.
硫化液和硅酸盐熔体中硒、碲的分配及其在硅酸盐土中的丰度
在地幔橄榄岩中观测到的硫(S)、硒(Se)和碲(Te)的近球粒陨石相对丰度已被用来支持原地球添加了碳质球粒陨石样晚饰面的假设。然而,观察到的S、Se和Te组成在多大程度上代表硅酸盐地球的特征仍然是一个争论的话题。在地幔源熔体(如洋中脊玄武岩)中Se和Te的浓度可以帮助我们对岩浆分异和地幔部分熔融过程中Se和Te的行为有一个精确的认识。本文通过室内实验确定了壳幔条件下硫化物液体硅酸盐熔体中Se和Te的分配系数(DSe,TeSul/Sil)。结果表明,Se的DSe、TeSul/Sil在180 ~ 2200之间,Te在1000 ~ 25400之间,与硅酸盐熔体中FeOtot含量呈倒u型关系。我们将DSe,TeSul/Sil参数化为硅酸盐熔体和硫化物液体组成的多功能,包括压力(0.5-2.5 GPa),温度(1273-1973 K)和氧逸度(FMQ-5至FMQ+1.5);FMQ指的是fayalite -磁铁矿-石英缓冲液,对DSe、TeSul/Sil的影响可以忽略不计。将我们的参数化方法应用于岩浆分异,可以有效地解释在morb和氧化弧岩浆中观察到的Se、Te和Cu的系统分布。更重要的是,与碳质球粒陨石相比,当应用于地幔部分熔融时,结合来自MORB的高精度Se和Te浓度数据,我们的参数化得到了枯竭MORB地幔和原始地幔的超球粒S/Se、S/Te和Se/Te比率。这些发现表明,硅酸盐土中的S、Se和Te丰度可能是在主要的吸积阶段建立的,而晚期的贴面只起了很小的作用。
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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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