RIMFAX Ground Penetrating Radar Reveals Dielectric Permittivity and Rock Density of Shallow Martian Subsurface
Author
Casademont, T.M.Eide, S.
Shoemaker, E.S.
Liu, Y.
Nunes, D.C.
Russell, P.
Dypvik, H.
Amundsen, H.E.F.
Berger, T.
Hamran, S.-E.
Affiliation
Lunar and Planetary Laboratory, University of ArizonaIssue Date
2023-03-21
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John Wiley and Sons IncCitation
Casademont, T. M., Eide, S., Shoemaker, E. S., Liu, Y., Nunes, D. C., Russell, P., et al. (2023). RIMFAX ground penetrating radar reveals dielectric permittivity and rock density of shallow Martian subsurface. Journal of Geophysical Research: Planets, 128, e2022JE007598. https://doi.org/10.1029/2022JE007598Rights
© 2023 The Authors. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial License.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The Mars 2020 Perseverance Rover is equipped with the RIMFAX ground penetrating radar instrument which has been continuously surveying the shallow subsurface during the rover's journey. Within the first 379 mission days, we identify hyperbolic patterns in the data, which are thought to be caused by objects such as buried boulders or cavities located in the upper 5 m of the subsurface. To obtain the first detailed estimates of radar wave propagation velocity, we match these scatterer-generated patterns with theoretical traveltime hyperbolas, which take into account the refraction at the surface. We employ these estimates to derive the average dielectric permittivity and bulk rock density of the volume above the scatterer source. The parameters compare well with those obtained through orbital radar measurements and those measured by other instruments onboard the Perseverance Rover. Our findings are consistent with a subsurface dominated by solid rock and mafic material. © 2023. The Authors.Note
Open access articleISSN
2169-9097Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1029/2022JE007598
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Except where otherwise noted, this item's license is described as © 2023 The Authors. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial License.