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Experimental investigation of the effect of nickel on the electrical resistivity of Fe-Ni and Fe-Ni-S alloys under pressure

  • Anne Pommier ORCID logo EMAIL logo
Published/Copyright: June 30, 2020
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Abstract

Electrical resistivity experiments were conducted on three alloys in the iron-rich side of the Fe-Ni(-S) system (Fe-5 wt% Ni, Fe-10 wt% Ni, Fe-10 wt% Ni-5 wt% S) at 4.5 and 8 GPa and up to 1900 K using the multi-anvil apparatus and the 4-electrode technique. For all samples, increasing temperature increases resistivity. At a specified temperature, Fe-Ni(-S) alloys are more resistive than Fe by a factor of about 3. Fe-Ni alloys containing 5 and 10 wt% Ni present comparable electrical resistivity values. The resistivity of Fe-Ni(-S) alloys is comparable to the one of Fe = 5 wt% S at 4.5 GPa and is about three times higher than the resistivity of Fe = 5 wt% S at 8 GPa, due to a different pressure dependence of electrical resistivity between Fe-Ni and Fe-S alloys. Based on these electrical results and experimentally determined thermal conductivity values from the literature, lower and upper bounds of thermal conductivity were calculated. For all Ni-bearing alloys, thermal conductivity estimates range between ~12 and 20 W/(m⋅K) over the considered pressure and temperature ranges. Adiabatic heat fluxes were computed for both Ganymede’s core and the Lunar core, and heat flux values suggest a significant dependence to both core composition and the adiabatic temperature. Comparison with previous thermochemical models of the cores of Ganymede and the Moon suggests that some studies may have overestimated the thermal conductivity and hence, the heat flux along the adiabat in these planetary cores.

Acknowledgments

Part of this work was performed while the author was invited professor at the Université de Lille, France. The author is grateful to Anne-Marie Blanchenet for her help with SEM analyses and Séverine Bellanger for microprobe analyses at the electron probe microanalyzer (EPMA) facility in Lille. Both are part of the ARCHI-CM project, supported by the Ministère de l’Enseignement Supérieur et de la Recherche, Région Nord-Pas de Calais and European Regional Development Fund (ERDF). A.P. also thanks Sébastien Merkel for hosting her during her stay in Lille, and Christopher Davies and James Badro for fruitful discussions. The author is grateful to Heather Watson for her conscientious editorial work and two Reviewers for their thorough comments that improved the manuscript.

  1. Funding

    This work was supported by NSF-CAREER grant 1750746 and NSF-NERC grant 1832462. Use of the COMPRES Cell Assembly Project was supported by COMPRES under NSF Cooperative Agreement EAR 1661511. The electrical cell used in these experiments is available via COMPRES.

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Received: 2019-09-25
Accepted: 2020-01-29
Published Online: 2020-06-30
Published in Print: 2020-07-28

© 2020 Walter de Gruyter GmbH, Berlin/Boston

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