The Effect of Salinity on Ocean Circulation and Ice–Ocean Interaction on Enceladus
Yaoxuan Zeng and Malte F. Jansen 2024 Planet. Sci. J. 5 13
The ice shell on Saturn’s moon Enceladus appears to be thicker at the equator that at the poles, which simulations suggest is due to a non-equilibrium state or tidal dissipation.