V
vogon13
Guest
I will admit to being somewhat out of step with ideas regarding the rapidity of the Iapetan coalesence from the primordially chaos.<br /><br />My analysis is that the proto-Iapetus may have been rather 'pokey' about sweeping up all the materials destined to be incorporated into itself. Considering the large volume these materials were distributed in, and Iapetus' rather pokey orbital velocity, I suspect Iapetus of being the solar system's slowest accreting major satellite, not one of it's fastest.<br /><br />In view of this, the decay heat of Al27 and other 'primoridal' isotopes was radiated from a vastly larger surface area of the proto-Iapetus and all the 'chunks'. Iapetus, in my view, is uniquely 'cold formed', among all the solar system objects. <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>