Enceladus already gets a significant amount of tidal heating due to its slightly egg-shape, and possibly if it had an eccentric orbit in its past.<br /><br />+++<br /><br />Finally, I wish to propose that if the interior of Enceladus is non-symmetrically inhomogeneous, that this in itself should be cause significant tidal heating. For example, if there was a lump of a high density material within the moon, but off-center, this should cause a very high amount of tidal heating, located above the dense lump.<br /><br />My hypothesis does not require that the lump itself offer radioactive heating, nor does it require that the lump carry remnant heat from a long-ago meteorite impact.<br /><br />Simply, if a dense large lump is present off-center in the moon, the lump will interact gravitationally with Dione, Saturn and other moons to cause the ices and rock above and around it to heat significantly due to unequal gravitatinal flexing. <div class="Discussion_UserSignature"> <div class="Discussion_UserSignature" align="center"><em><font color="#0000ff">- - - - - - - - - - - - - - - - - - - - - -</font></em> </div><div class="Discussion_UserSignature" align="center"><font color="#0000ff"><em>I really, really, really miss the "first unread post" function.</em></font> </div> </div>