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Dust grains generated by the Uranian irregular satellites will undergochaotic large-amplitude eccentricity oscillations under the simultaneous actionof radiation forces and the highly misaligned quadrupole potentials of theoblate planet and distant Sun. From a suite of orbital histories, we estimatecollision proba- bilities of dust particles with the regular satellites andargue that this process may explain the observed hemispherical colorasymmetries of the outermost four regular satellites of Uranus.

Chaotic dust dynamics and implications for the hemispherical color asymmetries of the Uranian satellites