Metal–silicate partitioning of sulphur, new experimental and thermodynamic constraints on planetary accretion

By A. Boujibar, D. Andrault, M. Bouhifd, N. Bolfan-Casanova, J. Devidal, N. Trcera. 2014

134 citations recorded by the source corpus.

Subfields: Geophysics

View Paper: https://www.semanticscholar.org/paper/255cb6ff183001daca00c7fbd47f138e76d20270

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In Geophysics

1. A. Morbidelli
2. T. O. S. University
3. Research School of Earth Sciences
4. D. Geology
5. T. Yoshizaki
6. William F. McDonough Department of Earth Science
7. L. Elkins‐Tanton
8. Japan.

Citations in the corpus

• The composition of Mars (2019, methodology): “The low S composition for the Martian core is supported by metal-silicate partition coefficients for S (Rose-Weston et al., 2009; Boujibar et al., 2014; Wang and Becker, 2017) and an experimental study of Fe isotopic fractionation under high pressure and temperature (Shahar et al.”
• The timeline of the lunar bombardment: Revisited (2018, methodology): “ initial S content, we rst calculate the S contents of mantle and core, immediately following lunar core formation, by mass balance using metal-silicate partition coecients for S as parameterized by Boujibar et al. (2014). Using the silicate melt composition of a fully molten LMO (Elkins-Tanton et a”