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Formation of Iapetus' Extreme Albedo Dichotomy by Exogenically Triggered Thermal Ice Migration

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Science  10 Dec 2009:
1177132
DOI: 10.1126/science.1177132

Abstract

The extreme albedo asymmetry of Saturn’s moon Iapetus, which is about 10 times brighter on its trailing hemisphere than on its leading hemisphere, has been an enigma for three centuries. Deposition of exogenic dark material on the leading side has been proposed as a cause, but cannot alone explain the global shape, sharpness and complexity of the transition between Iapetus’ bright and dark terrain. We demonstrate that all these characteristics, and the asymmetry’s large amplitude, can be plausibly explained by runaway global thermal migration of water ice, triggered by the deposition of dark material on the leading hemisphere. This mechanism is unique to Iapetus among the Saturnian satellites because its slow rotation produces unusually high daytime temperatures and H2O sublimation rates for a given albedo.