TY - JOUR
T1 - The high conductivity of iron and thermal evolution of the Earth's core
AU - Gomi, Hitoshi
AU - Ohta, Kenji
AU - Hirose, Kei
AU - Labrosse, Stéphane
AU - Caracas, Razvan
AU - Verstraete, Matthieu J.
AU - Hernlund, John W.
N1 - Funding Information:
We thank T. Komabayashi for discussions and Francis Nimmo and an anonymous reviewer for valuable comments. S.L. and R.C. are grateful to the LABEX Lyon Institute of Origins ( ANR-10-LABX-0066 ) of the Université de Lyon for its financial support within the program “Investissements d’Avenir” (ANR-11-IDEX-0007) of the French government operated par the National Research Agency (ANR). S.L. has been supported by the Agence Nationale de la Recherche under the grant ANR-08-JCJC-0084-01 . J.H. was supported by the National Science Foundation ( NSFEAR0855737 ).
PY - 2013/11
Y1 - 2013/11
N2 - We measured the electrical resistivity of iron and iron-silicon alloy to 100. GPa. The resistivity of iron was also calculated to core pressures. Combined with the first geophysical model accounting for saturation resistivity of core metal, the present results show that the thermal conductivity of the outermost core is greater than 90. W/m/K. These values are significantly higher than conventional estimates, implying rapid secular core cooling, an inner core younger than 1. Ga, and ubiquitous melting of the lowermost mantle during the early Earth. An enhanced conductivity with depth suppresses convection in the deep core, such that its center may have been stably stratified prior to the onset of inner core crystallization. A present heat flow in excess of 10. TW is likely required to explain the observed dynamo characteristics.
AB - We measured the electrical resistivity of iron and iron-silicon alloy to 100. GPa. The resistivity of iron was also calculated to core pressures. Combined with the first geophysical model accounting for saturation resistivity of core metal, the present results show that the thermal conductivity of the outermost core is greater than 90. W/m/K. These values are significantly higher than conventional estimates, implying rapid secular core cooling, an inner core younger than 1. Ga, and ubiquitous melting of the lowermost mantle during the early Earth. An enhanced conductivity with depth suppresses convection in the deep core, such that its center may have been stably stratified prior to the onset of inner core crystallization. A present heat flow in excess of 10. TW is likely required to explain the observed dynamo characteristics.
KW - Core
KW - Electrical resistivity
KW - High pressure
KW - Thermal conductivity
KW - Thermal evolution
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U2 - 10.1016/j.pepi.2013.07.010
DO - 10.1016/j.pepi.2013.07.010
M3 - Article
AN - SCOPUS:84886250789
SN - 0031-9201
VL - 224
SP - 88
EP - 103
JO - Physics of the Earth and Planetary Interiors
JF - Physics of the Earth and Planetary Interiors
ER -