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alexblackwell
Guest
<i>Guesses, anybody? ;-) Also, does anybody have any guesses about what new mysteries may be revealed? You've got just a few days before Cassini starts its closest study yet of the enigmatic moon, although I have no doubt that the mystery will linger for a long time to come.</i><br /><br />Some new Iapetus approach opnavs began hitting the ground yesterday, and the mystery deepens. See some of these processed images and discussion in Doug Ellison's Mars Exploration Rover Forum beginning on page 5 of a thread entitled "Iapetus Encounter In January."<br /><br />For review, below is the text from a slide in the Imaging Science Subsystem (ISS) presentation to the Cassini Satellites Orbiter Science Team (SOST) at the Iapetus B/C flyby preview meeting on December 20, 2004:<br /><br />=======================================<br /><br />About the [Iapetus] Albedo-Dichotomy Origin (table taken from [Tillman Denk's] DPS 2004 talk)<br /><br />Possible classification of Iapetus global albedo dichotomy origin hypotheses:<br /><br />1. Exogenic origin/ dust is coming in over long time<br /><br />(a) Dark grayish dust from Phoebe hits Iapetus's leading side and gets chemically altered/ reddened (Soter 1974, Burns et al. 1979, 1996; Hamilton 1997)<br /><br />(b) Dark reddish dust from smaller retrograde outer saturnian satellites covers Iapetus's leading side (Buratti et al. 2002)<br /><br />2. Asymmetric exogenic influence removes thin ice veneer from leading side, but not from trailing side and poles<br /><br />(a) Viewpoint of orbit mechanics:<br /><br />(a1) Circumsaturnian dust is the cause (from Phoebe or other outer Saturnian satellites)(Cruikshank et al. 1983; Bell et al. 1985; Buratti and Mosher 1995)<br /><br />(a2) Interplanetary micrometeoroid flux is the cause (Cook and Franklin 1970; Squyres and Sagan 1983; Wilson and Sagan 1996)<br /><br />(b) Viewpoint of physical processes on the surface:<br /><br />(b1) Exposing of the