http://arxiv.org/abs/1811.06536
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.
T. Hurford, W. Henning, R. Maguire, et. al.
Fri, 16 Nov 18
4/78
Comments: 31 pages, 5 pages, submitted to Icarus