  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.
