We propose a Cassini State model for Enceladus in which we assume the presence of a global ocean be- neath an ice shell and include the existence of defor- mations induced by obliquity tides. We aim to assess whether the obliquity of Enceladus can reach values large enough to trigger a strong heat flux caused by the dissipation associated with obliquity tides.
Baland, R.-M., Yseboodt, M., & Van Hoolst, T. (2015). Influence of the tides on the obliquity of Enceladus. European Planetary Science Congress, Nantes, France.