Host: The Japanese Society for Planetary Sciences: Local Organizing Committee for 2006 Fall Meeting
Europan visco-elastic tidal deformation due to its non-synchronous rotation is calculated. The relationship between the geological settings, the rotation period, and the surface rheology is investigated on the basis of this calculation. This investigation infers that the surface viscosity ranges between 1019 and 1020 Pa.s. The approach presented here suggests possibility of estimation for the surface viscosity on solid planets and satellites through its tectonic settings.