Matches in SemOpenAlex for { <https://semopenalex.org/work/W2518102166> ?p ?o ?g. }
- W2518102166 endingPage "138" @default.
- W2518102166 startingPage "123" @default.
- W2518102166 abstract "The highly siderophile elements (HSEs) are widely used as geochemical tracers for Earth’s accretion and core formation history. It is generally considered that core formation strongly depleted the Earth’s mantle in HSEs, which were subsequently replenished by a chondritic late veneer. However, open questions remain regarding the origin of suprachondritic Ru/Ir and Pd/Ir ratios that are thought to be characteristic for the primitive upper mantle. In most core-formation models that address the behavior of the HSEs, light elements such as S entering the core have not been taken into account and high P–T experimental data for S-bearing compositions are scarce. Here we present a comprehensive experimental study to investigate the effect of increasing S concentration in the metal on HSE metal–silicate partitioning at 2473 K and 11 GPa. We show that the HSEs become less siderophile with increasing S concentrations in the metal, rendering core-forming metal less efficient in removing the HSEs from the mantle if S is present. Furthermore, we investigated the FeS sulfide–silicate partitioning of the HSEs as a function of pressure (7–21 GPa) and temperature (2373–2673 K). The sulfide–silicate partition coefficient for Pt increases strongly with P, whereas those for Pd, Ru and Ir all decrease. The combined effect is such that above ∼20 GPa Ru becomes less chalcophile than Pt, which is opposite to their behavior in the metal–silicate system where Ru is always more siderophile than Pt. The newly determined experimental results are used in a simple 2-stage core formation model that takes into account the effect of S on the behavior of the HSEs during core formation. Results of this model show that segregation of a sulfide liquid to the core from a mantle with substantial HSE concentrations plays a key role in reproducing Earth’s mantle HSE abundances. As Ru and Pd are less chalcophile than Pt and Ir at high P–T, some Ru and Pd remain in the mantle after sulfide segregation. Addition of the late veneer then raised the concentrations of all HSE to their current levels. Suprachondritic Ru/Ir and Pd/Ir ratios of the mantle can thus be explained by a combination of sulfide segregation together with the addition of a late veneer without the need to invoke unknown chondritic material." @default.
- W2518102166 created "2016-09-16" @default.
- W2518102166 creator A5011538553 @default.
- W2518102166 creator A5016011747 @default.
- W2518102166 creator A5056591906 @default.
- W2518102166 creator A5077972151 @default.
- W2518102166 date "2016-12-01" @default.
- W2518102166 modified "2023-10-09" @default.
- W2518102166 title "The importance of sulfur for the behavior of highly-siderophile elements during Earth’s differentiation" @default.
- W2518102166 cites W1021473995 @default.
- W2518102166 cites W1409281717 @default.
- W2518102166 cites W1449351719 @default.
- W2518102166 cites W1796874662 @default.
- W2518102166 cites W1965598595 @default.
- W2518102166 cites W1969859799 @default.
- W2518102166 cites W1970207554 @default.
- W2518102166 cites W1970494800 @default.
- W2518102166 cites W1973220609 @default.
- W2518102166 cites W1974485318 @default.
- W2518102166 cites W1974703669 @default.
- W2518102166 cites W1981174654 @default.
- W2518102166 cites W1986120598 @default.
- W2518102166 cites W1988002846 @default.
- W2518102166 cites W1990613251 @default.
- W2518102166 cites W1991440717 @default.
- W2518102166 cites W1995798238 @default.
- W2518102166 cites W1997966853 @default.
- W2518102166 cites W2001333270 @default.
- W2518102166 cites W2001870274 @default.
- W2518102166 cites W2003143784 @default.
- W2518102166 cites W2003180371 @default.
- W2518102166 cites W2003733990 @default.
- W2518102166 cites W2004571857 @default.
- W2518102166 cites W2008937459 @default.
- W2518102166 cites W2010056906 @default.
- W2518102166 cites W2010659865 @default.
- W2518102166 cites W2014321303 @default.
- W2518102166 cites W2014413587 @default.
- W2518102166 cites W2015258641 @default.
- W2518102166 cites W2015537586 @default.
- W2518102166 cites W2016989256 @default.
- W2518102166 cites W2019037646 @default.
- W2518102166 cites W2020947023 @default.
- W2518102166 cites W2021677295 @default.
- W2518102166 cites W2022272868 @default.
- W2518102166 cites W2024997176 @default.
- W2518102166 cites W2026630163 @default.
- W2518102166 cites W2027609328 @default.
- W2518102166 cites W2027877967 @default.
- W2518102166 cites W2031103627 @default.
- W2518102166 cites W2034081712 @default.
- W2518102166 cites W2036786814 @default.
- W2518102166 cites W2037380844 @default.
- W2518102166 cites W2040161156 @default.
- W2518102166 cites W2041065531 @default.
- W2518102166 cites W2042369099 @default.
- W2518102166 cites W2043105337 @default.
- W2518102166 cites W2044377718 @default.
- W2518102166 cites W2045916826 @default.
- W2518102166 cites W2046310613 @default.
- W2518102166 cites W2050020771 @default.
- W2518102166 cites W2050246165 @default.
- W2518102166 cites W2056511558 @default.
- W2518102166 cites W2057306801 @default.
- W2518102166 cites W2058834305 @default.
- W2518102166 cites W2059651632 @default.
- W2518102166 cites W2059750087 @default.
- W2518102166 cites W2060783352 @default.
- W2518102166 cites W2061598985 @default.
- W2518102166 cites W2062049384 @default.
- W2518102166 cites W2063659395 @default.
- W2518102166 cites W2063809960 @default.
- W2518102166 cites W2065421390 @default.
- W2518102166 cites W2065783583 @default.
- W2518102166 cites W2070707331 @default.
- W2518102166 cites W2071397689 @default.
- W2518102166 cites W2073172102 @default.
- W2518102166 cites W2074014761 @default.
- W2518102166 cites W2077318864 @default.
- W2518102166 cites W2077364279 @default.
- W2518102166 cites W2079785352 @default.
- W2518102166 cites W2079958881 @default.
- W2518102166 cites W2080255100 @default.
- W2518102166 cites W2085064498 @default.
- W2518102166 cites W2085236573 @default.
- W2518102166 cites W2086545932 @default.
- W2518102166 cites W2087399346 @default.
- W2518102166 cites W2088516428 @default.
- W2518102166 cites W2089743632 @default.
- W2518102166 cites W2092264996 @default.
- W2518102166 cites W2092917902 @default.
- W2518102166 cites W2095245998 @default.
- W2518102166 cites W2095321171 @default.
- W2518102166 cites W2102148551 @default.
- W2518102166 cites W2108276901 @default.
- W2518102166 cites W2111696176 @default.
- W2518102166 cites W2119091455 @default.
- W2518102166 cites W2122131095 @default.