Vesalius (crater)

The outer rim of Vesalius is generally circular but somewhat irregular. There is an outward bulge at the southern extremity and a low rim at the northern end. The inner wall displays some slight terracing. On the interior floor the central peak is offset to the north, suggesting that the crater was formed by a low-angle impact.

Satellite craters

By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Vesalius. The name Eskola was proposed for Vesalius M crater, and it is shown as such in some publications, but the name was not approved by the IAU.