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 Earth and Planetary Science Letters Pub Date : 2025-02-24 DOI:10.1016/j.epsl.2025.119277
Zhiwei Liu , Yuan Li
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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.
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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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