Mike:
   I intend to
give a summary of the tidal forces and derive physical parameters
important in orbital evolution. For the latter half, I will go over the
Meyer and Wisdom paper (found here:
http://www.sciencedirect.com/science/article/pii/S0019103507004502) on the
tidal evolution of Mimas, Enceladus, and Dione, which shows how an
investigation into the orbital evolution of Saturn's moons can put
constraints on their physical parameters, i.e. their internal structures.

Dan:
I don't believe I need people to look at any paper other than this: http://www.nature.com/nature/journal/v470/n7332/pdf/nature09760.pdf