Crater degradation on Ceres is substantially more efficient than on the Moon despite a denser equilibrium crater population.
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A single mass flow event 600-1200 years ago formed the large smooth patch on comet 9P/Tempel 1, possibly triggered by Jupiter close encounters.
Multi-technique observations constrain the configuration of the ξ Tau system, detecting orbital oscillations on multiple timescales and suggesting component C is itself a binary.
citing papers explorer
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Degradation mechanisms and efficiency of heavily cratered regions on Ceres
Crater degradation on Ceres is substantially more efficient than on the Moon despite a denser equilibrium crater population.
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The Large Smooth Patch on Comet 9P/Tempel 1: Remnant of a Recent Past Event
A single mass flow event 600-1200 years ago formed the large smooth patch on comet 9P/Tempel 1, possibly triggered by Jupiter close encounters.
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Configuration of the $\xi$ Tau system constrained by multi-technique observations
Multi-technique observations constrain the configuration of the ξ Tau system, detecting orbital oscillations on multiple timescales and suggesting component C is itself a binary.