Montes Caucasus

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Detail map of Mare Imbrium's features. Montes Caucasus is marked "O".
Detail map of Mare Imbrium's features. Montes Caucasus is marked "O".
This article concerns the lunar mountain range. For other meanings, see Caucasus (disambiguation) and Caucasia (disambiguation).

Montes Caucasus is a rugged range of mountains in the northeastern part of the Moon. It begins at a gap of level surface that joins the Mare Imbrium to the west with the Mare Serenitatis to the east, and extends in an irregular band to the north-northeast to the western side of the prominent Eudoxus crater. The range forms the northwestern boundary of the Mare Serenitatis. It forms a continuation of the Montes Apenninus range to the southwest.

There are several breaks in the range where nearby lunar mare has intruded into the formation, particularly near the southern tip. Embedded within the eastern flank of the range is the Calippus crater. Along the eastern flank to the south of Eudoxus is the remnants of Alexander crater.

The selenographic coordinates of this range are 38.4° N, 10.0° E, and it has an official diameter of 445 km.[citation needed] However some observers list the length as being up to 550 km. The tallest peaks in this range reach heights of 6 km, undoubtedly providing an expansive view of the surroundings from their tops.

The range was named for the Caucasus Mountains on the Earth by the German selenographer Johann H. Mädler. However none of the peaks in this range have been assigned individual names, at least officially.

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