Walsh et al., 2011), water may have been delivered to the growing Earth and Mars in large quantities. The high metal/silicate partition coefficient of H found in recent experimental and computational works suggests that most of the water transported to our planet was sequestered mainly as up to ∼1 wt% H in the core (Li et al., 2020;Tagawa et al., 2021;Yuan & Steinle-Neumann, 2020). Indeed, H-bearing iron (Fe) alloys can explain the observed density and seismic-wave velocities in both the liquid outer core (Umemoto & Hirose, 2015, 2020) and the solid inner core (He et al., 2022;Wang et al., 2021). In addition, the recent marsquake observations by the InSight probe revealed that the Martian core is less dense than previously thought, possibly including 1-2 wt% H in addition to sulfur (S) (Stähler et al., 2021).The Fe-FeH phase diagram is of great importance to understand the present state and composition of planetary metallic cores. However, it is still vaguely known. Fe-H alloys must be examined under high pressure, because