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Water incorporation mechanisms and effects in MgSiO3-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 MgSiO3-majorite, which is a key end-member of majoritic garnet, at conditions up to 2000 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 MgSiO3-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 MgSiO3-majorite, which is opposite to that found for ringwoodite, offers a potential tool for investigating compositional heterogeneities in hydrated regions of planetary mantles.

Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1029/2025JB032448

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Earth Sciences
Role:
Author
ORCID:
0000-0003-3121-3255


Publisher:
Wiley
Journal:
Journal of Geophysical Research: Solid Earth More from this journal
Volume:
131
Issue:
1
Article number:
e2025JB032448
Publication date:
2025-12-26
Acceptance date:
2025-12-13
DOI:
EISSN:
2169-9356
ISSN:
2169-9313


Language:
English
Pubs id:
2350010
Local pid:
pubs:2350010
Deposit date:
2025-12-15
ARK identifier:

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