Good observations, TA.
Makes me wonder if maybe Iapetus has a
much higher fraction of organics in its crustal composition than the other icy moons. Something seems different about the surface's melt/freeze point behavior given the odd geometry of the craters. Alternatively (or, for that matter, possibly additionally), could there have been a significant global heating event
after the 'Snowman' and other major impact features were formed, such as tidal heating from orbital braking due to capture by Saturn?
Shooting from the hip, here: Iapetus seems more and more like an outer-system body out of place instead of a "native" Saturnian moon...NH may provide some interesting cross-reference data in 2015.
Admins, sorry for the OT excursion, but EC's montage rightly stimulates this line of discussion; please feel free to move to a suitable Iapetus thread!