Abstract

There is a considerable amount of literature on the electrical resistivity of iron at Earth’s core conditions, while only few studies have considered iron and iron-alloys at other planetary core conditions. Much of the total work has been carried out in the past decade and a review to collect data is timely. High pressures and temperatures can be achieved with direct measurements using a diamond-anvil cell, a multi-anvil press or shock compression methods. The results of direct measurements can be used in combination with first-principle calculations to extrapolate from laboratory temperature and pressure to the relevant planetary conditions. This review points out some discrepancies in the electrical resistivity values between theoretical and experimental studies, while highlighting the negligible differences arising from the selection of pressure and temperature values at planetary core conditions. Also, conversions of the reported electrical resistivity values to thermal conductivity via the Wiedemann-Franz law do not seem to vary significantly even when the Sommerfeld value of the Lorenz number is used in the conversion. A comparison of the rich literature of electrical resistivity values of pure Fe at Earth’s core-mantle boundary and inner-core boundary conditions with alloys of Fe and light elements (Si, S, O) does not reveal dramatic differences. The scarce literature on the electrical resistivity at the lunar core suggests the effect of P on a wt% basis is negligible when compared to that of Si and S. On the contrary, studies at Mercury’s core conditions suggest two distinct groups of electrical resistivity values but only a few studies apply to the inner-core boundary. The electrical resistivity values at the Martian core-mantle boundary conditions suggest a negligible contribution of Si, S and O. In contrast, Fe-S compositions at Ganymede’s core-mantle boundary conditions result in large deviations in electrical resistivity values compared to pure Fe. Contour maps of the reported values illustrate ρ(P, T) for pure Fe and its alloys with Ni, O and Si/S and allow for estimates of electrical resistivity at the core-mantle boundary and inner-core boundary conditions for the cores of terrestrial-like planetary bodies.

Highlights

  • The current interest in direct measurements and modelling of electrical resistivity (ρ) originates mainly from an interest in heat flow modelling of planetary cores

  • The differences in values for ρ at the Core-Mantle Boundary (CMB) reported from multi-anvil and Diamond-Anvil Cell (DAC) experimental studies may arise from uncertainties from large extrapolations, from predispositions specific to each method such as errors in sample geometries, temperature homogeneity of heated sample region, lack of sample symmetry, possible thermoelectric effects and other parasitic voltages, etc

  • The interest in determining qad is namely motivated by thermal evolution modelling

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Summary

INTRODUCTION

The current interest in direct measurements and modelling of electrical resistivity (ρ) originates mainly from an interest in heat flow modelling of planetary cores. While L > L0 for Fe-Si alloys at high T and low P (Secco, 2017), calculations at Earth core P, T conditions have shown that L < L0 (de Koker et al, 2012; Xu et al, 2018). Electrical resistivity is proportional to the inverse of the electron mean free path (d), which is proportional to the amplitudes of atomic vibrations (A) and proportional to T: FIGURE 1 | Cumulative number of publications on theoretical and experimental methods of estimating ρ of Fe, Fe-Ni, Fe-O and Fe-Si and S alloys at the core conditions of Earth, Moon, Mercury, Mars, and Ganymede. In Fe-alloys, the interaction of electron-lattice defects (including impurities) affects the scattering rate of conduction electrons. Bohnenkamp et al (2002) estimated a saturation value of 1.68 μΩm for Fe at 1 atm and up to 1,663 K, while there are variations in the saturation value of Fe-Si alloys at high P (Kiarasi and Secco, 2015; Gomi et al, 2016). Gomi et al (2013) were the first to propose the idea of resistivity saturation for Fe at Earth core conditions recent work (Zhang et al, 2020) provides contradictory results and suggests resistivity saturation behavior was an experimental artifact

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