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Author

H. Hussmann

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Open access Sep 2026

Underestimation of Planetary Contraction Due To Obscuration by Surface Roughness: The Case of Mercury

Estimating Mercury's radial contraction is key to understanding the planet's geodynamic evolution. Contraction has been inferred from mapped shortening structures, whose heterogeneous distribution contradicts the isotropic contraction expected from global cooling. Here we investigate the possibility that the tectonic r...

G. Nishiyama, A. Broquet, N. Tosi et al. · 1 citation
Preprint Aug 2026

Joint dynamical-geophysical evidence for a limit cycle in the Galilean moons

Io, Europa, and Ganymede orbit in the Laplace mean-motion resonance, where their orbital and thermochemical evolution are strongly coupled [1-5]. Forced eccentricities sustain tidal dissipation, powering Io's volcanism and maintaining Europa's subsurface ocean [6-8]. Tidal heating depends on the moons'eccentricities, s...

A. Bagheri, S. Vance, J. Fuller et al. · 0 citations

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