Tidal gravity data point to hot spot beneath Mars' crustal divide
Scientists modeled how Mars' gravity field shifts over time due to solar tides, using a technique that lets gravity harmonic coefficients vary periodically at annual, semi-annual and other frequencies within orbit-determination software. By tracking these small periodic gravity variations, they detected a thermal anomaly located beneath the boundary separating Mars' northern lowlands and southern highlands, known as the crustal dichotomy.
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This tidal tomography technique offers a new, indirect way to probe the interior structure and temperature of Mars without seismic instruments at that specific location. Finding a thermal anomaly under the dichotomy could help explain why Mars' crust split into two such different hemispheres, a mystery dating to the planet's early history.
- Researchers used time-varying spherical harmonic modeling of Mars' gravity field to study tidal responses.
- The analysis revealed a thermal anomaly beneath the boundary between Mars' northern and southern crustal regions.
- The method demonstrates how orbital gravity tracking can reveal deep interior features without direct seismic access.
Celestron NexStar 6SE Telescope — Mars science like this tidal tomography study starts with looking up — and the NexStar 6SE's computerized GoTo mount makes finding and tracking Mars simple for beginners. Its 6-inch Schmidt-Cassegrain optics reveal the planet's polar caps and dark surface markings, the same hemispheric contrasts researchers study from orbit.
See Celestron NexStar 6SE Telescope on Amazon → Affiliate link — we may earn a commission on purchases, at no extra cost to you. Product picked by AI based on this article; it is not a tested recommendation.Source: nature.com — Berne, 2026-08-26
Published there as: “Tidal tomography reveals a thermal anomaly beneath Mars’s crustal dichotomy”
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