[1] Its name was adopted by the International Astronomical Union (IAU) in 1976.

[2] A large irregular depression and several smaller ones are present in the southeastern part of the crater floor.

A similar depression is present in the crater Veronese which overlies the northwest rim of Mistral, and small ones are present in the unnamed crater to the southwest.

The depressions are similar to those within Navoi, Lermontov, Scarlatti, and Praxiteles.

This article about geology, geography or other features of the planet Mercury is a stub.