Subducting slabs play a crucial role in Earth’s water cycle. Hydrous minerals are important water carriers from the surface to the deep mantle in subducting slabs, and their physical properties are crucial to understanding the water cycle. Clinohumite [Mg9Si4O16(OH,F)2] is one of the main transformation products of serpentine under high pressure. As a member of the dense hydrous magnesium silicates (DHMSs), it is considered as a potential medium for water and other volatile components (e.g., fluorine) in subducting slabs to enter Earth’s deep interior. In this study, we measured the compressional (P) and shear (S) wave velocities of OH-clinohumite (Mg9Si4O18H2) at simultaneous pressure and temperature conditions up to 10 GPa and 873 K. Elastic properties were also obtained, yielding Ks0 = 114.4 (5) GPa, G0 = 75.2 (6) GPa, KS′ = 4.0 (1), G′ = 1.1 (1), ∂KS/∂T = −0.024 (1) GPa/K, and ∂G/∂T = −0.017 (2) GPa/K. Using these data, we calculated the density and wave velocity variations of harzburgite with different water contents under cold-slab upper-mantle conditions. We also discuss the effect of clinohumite with different XOH [OH/(F + OH) in molar] on the seismic wave velocities of cold or hot subducting slabs, and find that the wave velocity anomaly caused by clinohumite gradually decreases with increasing XOH. Seismic stratigraphic imaging across different subducting slabs reveals variations in velocity anomalies linked to clinohumite with differing hydroxyl (XOH) concentrations, allowing for the estimation of water fugacity within the subducting slab.
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Research Article|
June 16, 2025
Early Publication
Sound velocities of OH-clinohumite and implications for seismic velocities of hydrated subducting slab Available to Purchase
Baocun Wang;
Baocun Wang
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
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Nao Cai;
Nao Cai
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
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Duojun Wang;
Duojun Wang
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
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Junsheng Ma;
Junsheng Ma
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
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Rui Zhang;
Rui Zhang
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
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Peng Chen;
Peng Chen
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
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Kenan Han;
Kenan Han
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
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Chunyin Zhou;
Chunyin Zhou
2
Shanghai Synchrotron Radiation Facility, Shanghai Advanced Research Institute, Chinese Academy of Sciences, Shanghai 201210, China
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Ke Yang
Ke Yang
2
Shanghai Synchrotron Radiation Facility, Shanghai Advanced Research Institute, Chinese Academy of Sciences, Shanghai 201210, China
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Baocun Wang
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
Nao Cai
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
Duojun Wang
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
Junsheng Ma
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
Rui Zhang
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
Peng Chen
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
Kenan Han
1
High Pressure Science Experiment Center, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
Chunyin Zhou
2
Shanghai Synchrotron Radiation Facility, Shanghai Advanced Research Institute, Chinese Academy of Sciences, Shanghai 201210, China
Ke Yang
2
Shanghai Synchrotron Radiation Facility, Shanghai Advanced Research Institute, Chinese Academy of Sciences, Shanghai 201210, China
Publisher: Geological Society of America
Received:
11 Nov 2024
Revision Received:
16 Apr 2025
Accepted:
27 May 2025
First Online:
16 Jun 2025
Online ISSN: 1943-2674
Print ISSN: 0016-7606
© 2025 Geological Society of America
GSA Bulletin (2025)
Article history
Received:
11 Nov 2024
Revision Received:
16 Apr 2025
Accepted:
27 May 2025
First Online:
16 Jun 2025
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CitationBaocun Wang, Nao Cai, Duojun Wang, Junsheng Ma, Rui Zhang, Peng Chen, Kenan Han, Chunyin Zhou, Ke Yang; Sound velocities of OH-clinohumite and implications for seismic velocities of hydrated subducting slab. GSA Bulletin 2025; doi: https://doi.org/10.1130/B38132.1
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