TY - JOUR
T1 - Effects of iron on the lattice thermal conductivity of Earth’s deep mantle and implications for mantle dynamics
AU - Hsieh, Wen Pin
AU - Deschamps, Frédéric
AU - Okuchi, Takuo
AU - Lin, Jung Fu
N1 - Funding Information:
ACKNOWLEDGMENTS. We thank J. Yang, N. Tomioka, and S. Jacobsen for help with synthesis and preparation of the samples; S. Jacobsen for sharing experimental parameters for synthesis of ferropericlase and bridgmanite; and V. Prakapenka for his assistance with X-ray diffraction analysis of the starting crystals. The work by W.-P.H. and F.D. was supported by the Academia Sinica and Ministry of Science and Technology of Taiwan, Republic of China Contracts CDA-106-M02 (to W.-P.H.), MOST 103-2112-M-001-001-MY3 (to W.-P.H.), 105-2116-M-001-024 (to W.-P.H.), 106-2116-M-001-022 (to W.-P.H.), 105-2116-M-001-017 (to F.D.), and AS-102-CDA-M02 (to F.D.). J.-F.L. acknowledges support from the Geophysics and Cooperative Studies of the Earth’s Deep Interior Programs of the US National Science Foundation, the Visiting Professorship Program of the Institute for Planetary Materials, Okayama University, and the Center for High Pressure Science and Technology Advanced Research. This work was supported, in part, by Japan Society for the Promotion of Science KAKENHI Grant 26287135. X-ray diffraction patterns of the crystal were analyzed at GeoSoilEnviroCARS (GSECARS) sector of the Advanced Photon Source. GSECARS was supported by National Science Foundation Grant EAR-0622171 and Department of Energy Grant DE-FG02-94ER14466 under Contract DE-AC02-06CH11357. The APS is supported by 263 Department of Energy–Basic Energy Sciences Contract DE-AC02-06CH11357.
Funding Information:
We thank J. Yang, N. Tomioka, and S. Jacobsen for help with synthesis and preparation of the samples; S. Jacobsen for sharing experimental parameters for synthesis of ferropericlase and bridgmanite; and V. Prakapenka for his assistance with X-ray diffraction analysis of the starting crystals. The work by W.-P.H. and F.D. was supported by the Academia Sinica and Ministry of Science and Technology of Taiwan, Republic of China Contracts CDA-106-M02 (to W.-P.H.), MOST 103-2112-M-001-001-MY3 (to W.-P.H.), 105-2116-M-001-024 (to W.-P.H.), 106-2116-M-001-022 (to W.-P.H.), 105-2116-M-001-017 (to F.D.), and AS-102-CDA-M02 (to F.D.). J.-F.L. acknowledges support from the Geophysics and Cooperative Studies of the Earth’s Deep Interior Programs of the US National Science Foundation, the Visiting Professorship Program of the Institute for Planetary Materials, Okayama University, and the Center for High Pressure Science and Technology Advanced Research. This work was supported, in part, by Japan Society for the Promotion of Science KAKENHI Grant 26287135. X-ray diffraction patterns of the crystal were analyzed at GeoSoilEnviroCARS (GSECARS) sector of the Advanced Photon Source. GSECARS was supported by National Science Foundation Grant EAR-0622171 and Department of Energy Grant DE-FG02-94ER14466 under Contract DE-AC02-06CH11357. The APS is supported by 263 Department of Energy–Basic Energy Sciences Contract DE-AC02-06CH11357.
Publisher Copyright:
© 2018 National Academy of Sciences. All Rights Reserved.
PY - 2018/4/17
Y1 - 2018/4/17
N2 - Iron may critically influence the physical properties and thermochemical structures of Earth’s lower mantle. Its effects on thermal conductivity, with possible consequences on heat transfer and mantle dynamics, however, remain largely unknown. We measured the lattice thermal conductivity of lower-mantle ferropericlase to 120 GPa using the ultrafast optical pump-probe technique in a diamond anvil cell. The thermal conductivity of ferropericlase with 56% iron significantly drops by a factor of 1.8 across the spin transition around 53 GPa, while that with 8–10% iron increases monotonically with pressure, causing an enhanced iron substitution effect in the low-spin state. Combined with bridgmanite data, modeling of our results provides a self-consistent radial profile of lower-mantle thermal conductivity, which is dominated by pressure, temperature, and iron effects, and shows a twofold increase from top to bottom of the lower mantle. Such increase in thermal conductivity may delay the cooling of the core, while its decrease with iron content may enhance the dynamics of large low shear-wave velocity provinces. Our findings further show that, if hot and strongly enriched in iron, the seismic ultralow velocity zones have exceptionally low conductivity, thus delaying their cooling.
AB - Iron may critically influence the physical properties and thermochemical structures of Earth’s lower mantle. Its effects on thermal conductivity, with possible consequences on heat transfer and mantle dynamics, however, remain largely unknown. We measured the lattice thermal conductivity of lower-mantle ferropericlase to 120 GPa using the ultrafast optical pump-probe technique in a diamond anvil cell. The thermal conductivity of ferropericlase with 56% iron significantly drops by a factor of 1.8 across the spin transition around 53 GPa, while that with 8–10% iron increases monotonically with pressure, causing an enhanced iron substitution effect in the low-spin state. Combined with bridgmanite data, modeling of our results provides a self-consistent radial profile of lower-mantle thermal conductivity, which is dominated by pressure, temperature, and iron effects, and shows a twofold increase from top to bottom of the lower mantle. Such increase in thermal conductivity may delay the cooling of the core, while its decrease with iron content may enhance the dynamics of large low shear-wave velocity provinces. Our findings further show that, if hot and strongly enriched in iron, the seismic ultralow velocity zones have exceptionally low conductivity, thus delaying their cooling.
KW - E
KW - Ferropericlase
KW - Geodynamics
KW - Large low shear-wave
KW - Thermal conductivity
KW - Ultralow velocity zones
KW - Velocity provinces
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U2 - 10.1073/pnas.1718557115
DO - 10.1073/pnas.1718557115
M3 - Article
C2 - 29610319
AN - SCOPUS:85045517833
SN - 0027-8424
VL - 115
SP - 4099
EP - 4104
JO - Proceedings of the National Academy of Sciences of the United States of America
JF - Proceedings of the National Academy of Sciences of the United States of America
IS - 16
ER -