Seasonal Variations of Soil Thermal Conductivity at the InSight Landing Site

Author:

Grott M.1ORCID,Piqueux S.2ORCID,Spohn T.13ORCID,Knollenberg J.1,Krause C.4,Marteau E.2ORCID,Hudson T. L.2ORCID,Forget F.5,Lange L.5ORCID,Müller N.1,Golombek M.2,Nagihara S.6ORCID,Morgan P.7ORCID,Murphy J. P.8,Siegler M.910ORCID,King S. D.8ORCID,Banfield D.11,Smrekar S. E.2,Banerdt W. B.2ORCID

Affiliation:

1. German Aerospace Center (DLR) Institute of Planetary Research Berlin Germany

2. Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA

3. International Space Science Institute (ISSI) Bern Switzerland

4. German Aerospace Center (DLR) MUSC Space Operations and Astronaut Training Cologne Germany

5. Laboratoire de Météorologie Dynamique (LMD/IPSL/CNRS) Sorbonne Université Paris France

6. Department of Geosciences Texas Tech University Lubbock TX USA

7. Colorado Geological Survey Colorado School of Mines Golden CO USA

8. Virginia Polytechnic Institute and State University Blacksburg VA USA

9. Planetary Science Institute Tucson AZ USA

10. Southern Methodist University Dallas TX USA

11. Cornell University Ithaca NY USA

Abstract

AbstractThe heat flow and physical properties package measured soil thermal conductivity at the landing site in the 0.03–0.37 m depth range. Six measurements spanning solar longitudes from 8.0° to 210.0° were made and atmospheric pressure at the site was simultaneously measured using InSight's Pressure Sensor. We find that soil thermal conductivity strongly correlates with atmospheric pressure. This trend is compatible with predictions of the pressure dependence of thermal conductivity for unconsolidated soils under martian atmospheric conditions, indicating that heat transport through the pore filling gas is a major contributor to the total heat transport. Therefore, any cementation or induration of the soil sampled by the experiments must be minimal and soil surrounding the mole at depths below the duricrust is likely unconsolidated. Thermal conductivity data presented here are the first direct evidence that the atmosphere interacts with the top most meter of material on Mars.

Funder

Jet Propulsion Laboratory

Deutsches Zentrum für Luft- und Raumfahrt

National Aeronautics and Space Administration

Österreichischen Akademie der Wissenschaften

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

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