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At high resolution, terrain in the transition region between bright and dark hemispheres on Saturn's moon Iapetus reveals a spotty appearance reminiscent of a Dalmatian. The bright material on the frozen surface of Iapetus, 1,468 kilometers (912 miles) across, is water ice, and the dark material is likely carbonaceous in composition. The dark material is preferentially found at the bottoms of craters. Bright water ice forms the "bed rock" on Iapetus, while the dark, presumably loose material apparently lies on top of the ice. The terrain seen here is also visible in

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      EUN,LOM,LRE4,hdl:10494/259292,work-cmr-id:259292,http://photojournal.jpl.nasa.gov:http://photojournal.jpl.nasa.gov/catalog/PIA08382,ilox,learning resource exchange,LRE metadata application profile,LRE

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