Our knowledge of the structure and composition of Earth's core is based on sparse direct evidence (e.g., from seismology, geodesy, geo-and paleo-magnetism) and many indirect observations (from cosmochemistry, experimental petrology, and mineral physics) (Allègre et al., 1995;McDonough & Sun, 1995). Cosmochemical studies on iron meteorites and a comparison of mineral physics data with seismological observations (measurements of density (ρ) and compressional (V P ) and shear (V S ) wave velocities under extreme conditions) suggest that Earth's inner core is primarily composed of metallic Fe-Ni alloy (5-25 wt.% Ni) (McDonough & Sun, 1995;Wasson & Chou, 1974). However, the inner core density is ∼5 % lower than pure Fe at corresponding pressures and temperatures (Dewaele et al., 2006;Fei et al., 2016), presumably due to the presence of light elements (Birch, 1952) that were incorporated in the core during its formation (