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Zhao Y, Wu Z, Hao S, Wang W, Deng X, Song J. Elastic properties of Fe-bearing Akimotoite at mantle conditions: Implications for composition and temperature in lower mantle transition zone. FUNDAMENTAL RESEARCH 2022; 2:570-577. [PMID: 38934001 PMCID: PMC11197629 DOI: 10.1016/j.fmre.2021.12.013] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/09/2021] [Revised: 11/18/2021] [Accepted: 12/21/2021] [Indexed: 11/18/2022] Open
Abstract
The pyrolite model, which can reproduce the upper-mantle seismic velocity and density profiles, was suggested to have significantly lower velocities and density than seismic models in the lower mantle transition zone (MTZ). This argument has been taken as mineral-physics evidence for a compositionally distinct lower MTZ. However, previous studies only estimated the pyrolite velocities and density along a one-dimension (1D) geotherm and never considered the effect of lateral temperature heterogeneity. Because the majorite-perovskite-akimotoite triple point is close to the normal mantle geotherm in the lower MTZ, the lateral low-temperature anomaly can result in the presence of a significant fraction of akimotoite in pyrolitic lower MTZ. In this study, we reported the elastic properties of Fe-bearing akimotoite based on first-principles calculations. Combining with literature data, we found that the seismic velocities and density of the pyrolite model can match well those in the lower MTZ when the lateral temperature heterogeneity is modeled by a Gaussian distribution with a standard deviation of ∼100 K and an average temperature of dozens of K higher than the triple point of MgSiO3. We suggest that a harzburgite-rich lower MTZ is not required and the whole mantle convection is expected to be more favorable globally.
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Affiliation(s)
- Yajie Zhao
- Laboratory of Seismic and Physics of Earth's Interior, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China
| | - Zhongqing Wu
- Laboratory of Seismic and Physics of Earth's Interior, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China
- National Geophysical Observatory at Mengcheng, University of Science and Technology of China, Hefei, China
- CAS Center for Excellence in Comparative Planetology, USTC, Hefei 230026, China
| | - Shangqin Hao
- Laboratory of Seismic and Physics of Earth's Interior, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China
- Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California San Diego, La Jolla 92092, CA, USA
| | - Wenzhong Wang
- Department of Earth Sciences, University College London, London WC1E 6BT, United Kingdom
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA
| | - Xin Deng
- Laboratory of Seismic and Physics of Earth's Interior, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China
| | - Jian Song
- Laboratory of Seismic and Physics of Earth's Interior, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China
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First Principles Thermodynamics of Minerals at HP–HT Conditions: MgO as a Prototypical Material. MINERALS 2017. [DOI: 10.3390/min7100183] [Citation(s) in RCA: 19] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 01/23/2023]
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Ballmer MD, Schmerr NC, Nakagawa T, Ritsema J. Compositional mantle layering revealed by slab stagnation at ~1000-km depth. SCIENCE ADVANCES 2015; 1:e1500815. [PMID: 26824060 PMCID: PMC4730845 DOI: 10.1126/sciadv.1500815] [Citation(s) in RCA: 16] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/22/2015] [Accepted: 09/21/2015] [Indexed: 06/02/2023]
Abstract
Improved constraints on lower-mantle composition are fundamental to understand the accretion, differentiation, and thermochemical evolution of our planet. Cosmochemical arguments indicate that lower-mantle rocks may be enriched in Si relative to upper-mantle pyrolite, whereas seismic tomography images suggest whole-mantle convection and hence appear to imply efficient mantle mixing. This study reconciles cosmochemical and geophysical constraints using the stagnation of some slab segments at ~1000-km depth as the key observation. Through numerical modeling of subduction, we show that lower-mantle enrichment in intrinsically dense basaltic lithologies can render slabs neutrally buoyant in the uppermost lower mantle. Slab stagnation (at depths of ~660 and ~1000 km) and unimpeded slab sinking to great depths can coexist if the basalt fraction is ~8% higher in the lower mantle than in the upper mantle, equivalent to a lower-mantle Mg/Si of ~1.18. Global-scale geodynamic models demonstrate that such a moderate compositional gradient across the mantle can persist can in the presence of whole-mantle convection.
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Affiliation(s)
- Maxim D. Ballmer
- Earth-Life Science Institute, Tokyo Institute of Technology, Tokyo 152-8551, Japan
- School of Ocean and Earth Sciences and Technology, University of Hawaii at Manoa, Honolulu, HI 96822, USA
| | | | - Takashi Nakagawa
- Department of Mathematical Science and Advanced Technology, Japan Agency for Marine-Earth Science and Technology, Yokohama 236-0001, Japan
| | - Jeroen Ritsema
- Department of Earth and Environmental Sciences, University of Michigan, Ann Arbor, MI 48109, USA
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Affiliation(s)
- Barbara Romanowicz
- Berkeley Seismological Laboratory and Department of Earth and Planetary Science, University of California at Berkeley, Berkeley, CA 94720, USA
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Duffy TS. Some recent advances in understanding the mineralogy of Earth's deep mantle. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2008; 366:4273-4293. [PMID: 18826921 DOI: 10.1098/rsta.2008.0172] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/26/2023]
Abstract
Understanding planetary structure and evolution requires a detailed knowledge of the properties of geological materials under the conditions of deep planetary interiors. Experiments under the extreme pressure-temperature conditions of the deep mantle are challenging, and many fundamental properties remain poorly constrained or are inferred only through uncertain extrapolations from lower pressure-temperature states. Nevertheless, the last several years have witnessed a number of new developments in this area, and a broad overview of the current understanding of the Earth's lower mantle is presented here. Some recent experimental and theoretical advances related to the lowermost mantle are highlighted. Measurements of the equation of state and deformation behaviour of (Mg,Fe)SiO3 in the CaIrO3-type (post-perovskite) structure yield insights into the nature of the core-mantle boundary region. Theoretical studies of the behaviour of MgSiO3 liquids under high pressure-temperature conditions provide constraints on melt volumes, diffusivities and viscosities that are relevant to understanding both the early Earth (e.g. deep magma oceans) and seismic structure observed in the present Earth (e.g. ultra-low-velocity zones).
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Affiliation(s)
- Thomas S Duffy
- Department of Geosciences, Princeton University, Princeton, NJ 08544, USA.
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