Ceres and the terrestrial planets impact cratering record

@article{Strom2018CeresAT,
  title={Ceres and the terrestrial planets impact cratering record},
  author={Robert Strom and Simone Marchi and Renu Malhotra},
  journal={Icarus},
  year={2018},
  volume={302},
  pages={104-108}
}
Abstract Dwarf planet Ceres, the largest object in the Main Asteroid Belt, has a surface that exhibits a range of crater densities for a crater diameter range of 5–300 km. In all areas the shape of the craters’ size-frequency distribution is very similar to those of the most ancient heavily cratered surfaces on the terrestrial planets. The most heavily cratered terrain on Ceres covers ∼15% of its surface and has a crater density similar to the highest crater density on 

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Data and Techniques

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