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arxiv: 1811.06536 · v1 · pith:AH6F2IJLnew · submitted 2018-11-15 · 🌌 astro-ph.EP

Seismicity on Tidally Active Solid-Surface Worlds

classification 🌌 astro-ph.EP
keywords energybodiesseismictidalactiveactivitydescribedissipate
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Tidal interactions between planets or stars and the bodies that orbit them dissipate energy in their interiors. The energy dissipated drives internal heating and a fraction of that energy will be released as seismic energy. Here we formalize a model to describe the tidally-driven seismic activity on planetary bodies based on tidal dissipation.

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    Coupled Lorentz-tide simulations show cores with dynamic viscosity above ~10^24 Pa s can survive over 1 Gyr in kilogauss magnetic fields around white dwarfs.