Compositional and thermal state of the lower mantle from joint 3D inversion with seismic tomography and mineral elasticity

Author:

Deng Xin1ORCID,Xu Yinhan1,Hao Shangqin12ORCID,Ruan Youyi34,Zhao Yajie1ORCID,Wang Wenzhong156,Ni Sidao7,Wu Zhongqing156ORCID

Affiliation:

1. Deep Space Exploration Laboratory / School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China

2. Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California San Diego, La Jolla, CA 92092

3. School of Earth Sciences and Engineering, Nanjing University, Nanjing, Jiangsu 210023, China

4. Institute of Earth Exploration and Sensing, Nanjing University, Nanjing, Jiangsu 210023, China

5. Chinese Academy of Sciences, Center for Excellence in Comparative Planetology, University of Science and Technology of China, Hefei, Anhui 233500, China

6. National Geophysical Observatory at Mengcheng, University of Science and Technology of China, Hefei, Anhui 233500, China

7. State Key Laboratory of Geodesy and Earth’s Dynamics, Innovation Academy for Precision Measurement Science and Technology, Chinese Academy of Sciences, Wuhan, Hubei 430077, China

Abstract

The compositional and thermal state of Earth’s mantle provides critical constraints on the origin, evolution, and dynamics of Earth. However, the chemical composition and thermal structure of the lower mantle are still poorly understood. Particularly, the nature and origin of the two large low-shear-velocity provinces (LLSVPs) in the lowermost mantle observed from seismological studies are still debated. In this study, we inverted for the 3D chemical composition and thermal state of the lower mantle based on seismic tomography and mineral elasticity data by employing a Markov chain Monte Carlo framework. The results show a silica-enriched lower mantle with a Mg/Si ratio less than ~1.16, lower than that of the pyrolitic upper mantle (Mg/Si = 1.3). The lateral temperature distributions can be described by a Gaussian distribution with a standard deviation (SD) of 120 to 140 K at 800 to 1,600 km and the SD increases to 250 K at 2,200 km depth. However, the lateral distribution in the lowermost mantle does not follow the Gaussian distribution. We found that the velocity heterogeneities in the upper lower mantle mainly result from thermal anomalies, while those in the lowermost mantle mainly result from compositional or phase variations. The LLSVPs have higher density at the base and lower density above the depth of ~2,700 km than the ambient mantle, respectively. The LLSVPs are found to have ~500 K higher temperature, higher Bridgmanite and iron content than the ambient mantle, supporting the hypothesis that the LLSVPs may originate from an ancient basal magma ocean formed in Earth’s early history.

Funder

Strategic Priority Research Program (B) of the Chinese Academy of Sciences

MOST | National Natural Science Foundation of China

MOE | Fundamental Research Funds for the Central Universities

Publisher

Proceedings of the National Academy of Sciences

Subject

Multidisciplinary

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