Collisional and dynamical models indicate the Eulalia parent body disruption ~800 Ma near the J3:1 resonance produced an impact shower that accounts for observed lunar craters formed near that time.
J., Antonenko, I., Kirchoff, M
2 Pith papers cite this work. Polarity classification is still indexing.
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Crater degradation on Ceres is substantially more efficient than on the Moon despite a denser equilibrium crater population.
citing papers explorer
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An 800-Million-Year-Old Impact Shower on the Terrestrial Planets from the Breakup of the Eulalia Parent Body
Collisional and dynamical models indicate the Eulalia parent body disruption ~800 Ma near the J3:1 resonance produced an impact shower that accounts for observed lunar craters formed near that time.
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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.