V
vogon13
Guest
I have noted that tidal effects between the earth and moon are manifest primarily in the familar ocean tides, and less familiarly, in dissipation of the (resonably) solid body of our planet.<br /><br />Also, that the tidal interaction between Jupiter and Io is manifested in dissipation in Jupiters atmosphere.<br /><br />I have been considering tidal interactions (non-mathematically, so far) between icy moons and their possible satellites.<br /><br />Recent spacecraft missions have shown small bodies around the solar system to be structured quite amazingly. Loosely compacted granular materials seem to be the favored model now. Such objects seem to be amazingly resilient to (large) impact damage. This really shows just how different their internal structure is.<br /><br />My question:<br /><br />How do tidal effects manifest themselves in such objects?<br /><br />Do they dissipate as easily as a gas or liquid? Are their porosities affected? Does flexing of the object reveal itself in any particular pattern in the surface we might examine? Do such objects rapidly evolve their orbits tidally when in proximity to other objects, or slowly? Are there any trends we might observe in tidally mature systems?<br /><br />Jes' curious!<br /><br /> <div class="Discussion_UserSignature"> <p><font color="#ff0000"><strong>TPTB went to Dallas and all I got was Plucked !!</strong></font></p><p><font color="#339966"><strong>So many people, so few recipes !!</strong></font></p><p><font color="#0000ff"><strong>Let's clean up this stinkhole !!</strong></font> </p> </div>