Water Incorporation Mechanisms and Effects in MgSiO ₃ ‐Majorite Under High Temperature and Pressure Conditions

Abstract The incorporation of water in high‐pressure minerals is essential for the water cycle within the interiors of terrestrial planets. Majoritic garnet, a major component in the mantles of Earth and Mars, plays a significant role in this context. In this study, we use first‐principles simulations to explore water incorporation mechanisms in MgSiO 3 ‐majorite, which is a key end‐member of majoritic garnet, at conditions up to 2,000 K and 20 GPa. By dealing with the relationship between chemical potential and the Gibbs free energy changes for the reactions at equilibrium conditions, we determine the ratios of the seven potential hydrous defects. Our results reveal that the Si2 and Si3 defects, which are of the hydrogarnet‐type, dominate water incorporation in MgSiO 3 ‐majorite. In addition, we evaluate the effects of these hydrous defects on seismic wave velocities. The presence of Si2 and Si3 defects, with an expected water concentration of ∼700 ppm, has a small effect on both P‐wave and S‐wave velocities. Nevertheless, the influence of water on lateral variations in the seismic wave velocities of MgSiO 3 ‐majorite, which is opposite to that found for ringwoodite, offers a potential tool for investigating compositional heterogeneities in hydrated regions of planetary mantles.