We study the translational oscillation modes of the interior of large icy satellites such as Titan, Europa, Callisto and Ganymede. The observation of these modes could allow constraining the interior structure of icy satellites and in particular the ocean thickness.
Coyette, A., & Van Hoolst, T. (2013). Slichter modes of large icy satellites. European Planetary Science Congress 2013, Londres. https://hdl.handle.net/2078.5/35258