Seismicity on Tidally Active Solid-Surface Worlds

T. A. Hurford; W. G. Henning; R. Maguire; V. Lekic; N. Schmerr; M. Panning; V. J. Bray; M. Manga; S. A. Kattenhorn; L. C. Quick; A. R. Rhoden

arXiv · 1811.06536

Seismicity on Tidally Active Solid-Surface Worlds

T. A. Hurford·W. G. Henning·R. Maguire·V. Lekic·N. Schmerr·M. Panning·V. J. Bray·M. Manga·S. A. Kattenhorn·L. C. Quick·A. R. Rhoden

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Abstract

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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T. A. Hurford, W. G. Henning, R. Maguire, V. Lekic, N. Schmerr, M. Panning, V. J. Bray, M. Manga, S. A. Kattenhorn, L. C. Quick, A. R. Rhoden. 2018-11-15. Seismicity on Tidally Active Solid-Surface Worlds. https://arxiv.org/abs/1811.06536

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