Where a crater formation has associated satellite craters, these are detailed on the main crater description pages.

This crater formation has been heavily worn and eroded by impact erosion.

The results were inconclusive, but not inconsistent with the estimated 800 million year age of crater formation.

Observations in the walls of the pit craters indicate that there have been several episodes of cone and pit crater formation.

The fact that we know when their surfaces were formed will also be useful in determining the rate of crater formation in asteroids.