Tidal tomography reveals a thermal anomaly beneath Mars’s crustal dichotomy

Abstract Mars undergoes seasonal tidal forcing as a result of its eccentric orbit and the tilt of its rotation axis relative to the Sun 1 . Response to this forcing produces temporal variations in the Martian gravity field and is sensitive to the internal structure of the planet 2–4 . Using tracking data from the Mars Global Surveyor (MGS), Mars Odyssey (ODY) and Mars Reconnaissance Orbiter (MRO) spacecraft 5–7 , we demonstrate that degree-3 components of the time-variable gravity field of Mars differ by up to 300% from predictions for a spherically symmetric planet 8–10 . These deviations can be explained if the effective shear modulus of the mantle varies by >20% over a roughly north–south pattern that closely aligns with the surface expression of the Martian crustal dichotomy 11 . On the basis of this correlation, we infer preservation of a 200–400 °C thermal anomaly in the present-day mantle below the southern highlands of Mars. This temperature variation could reflect regional mantle convection 12,13 or insulation by the thick southern highlands crust of Mars that has persisted over several billion years 14,15 .

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Publication Details

Journal
Nature
Published
2026-08-26
DOI
https://doi.org/10.1038/s41586-026-10893-x
Primary Topic
Planetary Science and Exploration
Type
article
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article

Tidal tomography reveals a thermal anomaly beneath Mars’s crustal dichotomy

D. Hemingway, Sander Goossens, Angela G. Marusiak, I. Matsuyama et al.
Nature
Planetary Science and Exploration
article

Tidal tomography reveals a thermal anomaly beneath Mars’s crustal dichotomy

D. Hemingway, Sander Goossens, Angela G. Marusiak, I. Matsuyama, Shijie Zhong, Marc Rovira‐Navarro, H. C. P. Lau, Alexander Berne, Nick Wagner, F. Nimmo, Antonio Genova, Kar Wai Cheng, Chuan Qin, Amirhossein Bagheri
article en

Abstract

Abstract Mars undergoes seasonal tidal forcing as a result of its eccentric orbit and the tilt of its rotation axis relative to the Sun 1 . Response to this forcing produces temporal variations in the Martian gravity field and is sensitive to the internal structure of the planet 2–4 . Using tracking data from the Mars Global Surveyor (MGS), Mars Odyssey (ODY) and Mars Reconnaissance Orbiter (MRO) spacecraft 5–7 , we demonstrate that degree-3 components of the time-variable gravity field of Mars differ by up to 300% from predictions for a spherically symmetric planet 8–10 . These deviations can be explained if the effective shear modulus of the mantle varies by >20% over a roughly north–south pattern that closely aligns with the surface expression of the Martian crustal dichotomy 11 . On the basis of this correlation, we infer preservation of a 200–400 °C thermal anomaly in the present-day mantle below the southern highlands of Mars. This temperature variation could reflect regional mantle convection 12,13 or insulation by the thick southern highlands crust of Mars that has persisted over several billion years 14,15 .

NatureVol. 656(8129)
California Institute of Technology (US), Planetary Science Institute (US), Goddard Space Flight Center (US), University of Arizona (US), University of California, Los Angeles (US), University of California, Santa Cruz (US), University of Colorado Boulder (US), Brown University (US), Institute of Earth Sciences, Academia Sinica (TW), Sapienza University of Rome (IT), The University of Texas at Austin (US), Delft University of Technology (NL)
Life below water
Openalex Percentile: Top 10%
Planetary Science and Exploration
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