Sulfur saturation limits in silicate melts and their implications for core formation scenarios for terrestrial planets

By A. Holzheid, T. Grove. 2002

193 citations recorded by the source corpus.

Subfields: Geophysics

View Paper: https://www.semanticscholar.org/paper/9fc1f850cd62e39fb6ce60c5b037d435294194e5

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Geophysics

1. F. Gaillard
2. Bruno Scaillet

Citations in the corpus

• Is Mercury a volatile‐rich planet? (2012, unknown): “Based on available experimental data for S solubility in silicate liquids [Beermann et al., 2011; Berthet et al., 2009; Holzheid and Grove, 2002; Malavergne et al., 2007a; Mavrogenes and O’Neill, 1999; McCoy et al., 1999; Moune et al., 2009], and assuming the sulfur abundances at the Mercurian…”
• The sulfur content of volcanic gases on Mars (2009, background): “There is a continuous miscibility between S-free molten iron and molten FeS (Kress, 1997) that is however characterized by important deviations from ideal behavior (Wang et al., 1991, see Supplementary materials, SM in the Appendix).”