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arXiv · 1804.01229

Ceres and the Terrestrial Planets Impact Cratering Record

Robert G. Strom·Simone Marchi·Renu Malhotra
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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 <1% of the lunar highlands. This region of higher crater density on Ceres probably records the high impact rate at early times and indicates that the other 85% of Ceres was partly resurfaced after the Late Heavy Bombardment (LHB) at ~4 Ga. The Ceres cratering record strongly indicates that the period of Late Heavy Bombardment originated from an impactor population whose size-frequency distribution resembles that of the Main Belt Asteroids.

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Robert G. Strom, Simone Marchi, Renu Malhotra. 2018-04-04. Ceres and the Terrestrial Planets Impact Cratering Record. https://doi.org/10.1016/j.icarus.2017.11.013

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