Thin-shell Tidal Dynamics of Ocean Worlds

Thin-shell Tidal Dynamics of Ocean Worlds

Several solar system moons harbor subsurface water oceans; extreme internal heating or solar irradiation can form magma oceans in terrestrial bodies. Tidal forces drive ocean currents, producing tidal heating that affects the thermal−orbital evolution of these worlds. If the outermost layers (ocean...

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Bibliographic Details
Main Authors:	Marc Rovira-Navarro, Isamu Matsuyama, Hamish C. F. C Hay
Format:	Article
Language:	English
Published:	IOP Publishing 2023-01-01
Series:	The Planetary Science Journal
Subjects:	Ocean tides Natural satellites (Solar system) Earth-moon system Io Enceladus
Online Access:	https://doi.org/10.3847/PSJ/acae9a

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