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Reaction between Hydrogen and Ferrous/Ferric Oxides at High Pressures and High Temperatures—Implications for Sub-Neptunes and Super-Earths

  • Authors: H. W. Horn, V. Prakapenka, S. Chariton, S. Speziale, S.-H. Shim

H. W. Horn et al 2023 The Planetary Science Journal 4 .

  • Provider: AAS Journals

Caption: Figure 2.

X-ray diffraction patterns from run Hem-4 (Table 1) taken at 38 GPa (a) before heating, (b) during heating (∼1850 K), and (c) after heating. The upper pattern in panel (b) is during the first heating event, and the lower pattern is during the final heating event. The vertical tick marks below each integrated diffraction pattern represent the diffraction peak positions of the various observed mineral phases. Expected peak positions are calculated by combining the experimentally determined crystal structure and equation of state for a given material. Initially both FeO and FeH x were formed, but after four heating events only FeH x was observed in diffraction patterns.

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