|Colongitude||329° at sunrise|
|Eponym||Marcus P. Vitruvius|
Vitruvius is a small lunar impact crater that lies on the northern edge of the Mare Tranquillitatis. Less than 90 km north is the crater Littrow, about 45 km northwest is Fabbroni, about 48 km east is Gardner and 53 km southwest is Beketov. About 35 km north-northwest is the elongated Mons Vitruvius mountain, and beyond is the valley where the Apollo 17 mission landed. Also south is Dorsa Barlow (Barlow Hills), further southeast is Mons Esam (Esam Mountains).
The crater is named after the great Roman engineer and architect Marcus P. Vitruvius.
Its diameter is 30 km long and is 1,880 meters deep. The area is between 675 and 700 km² and the perimeter is less than 100 km.
The rim of Vitruvius is somewhat circular, but the sides are uneven to the north and east. The rim is highest to the northwest. The interior floor is uneven, with some low rises in the southwest. A small crater is attached to southern outer rim. The surroundings grow more rugged to the north of the crater.
By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Vitruvius.
|B||16.4° N||33.0° E||18 km|
|G||13.9° N||34.6° E||6 km|
|H||16.4° N||33.9° E||22 km|
|L||19.0° N||30.7° E||6 km|
|M||16.1° N||31.5° E||5 km|
|T||17.1° N||33.2° E||15 km|
The following craters have been renamed by the IAU.
View of the Earth
Being located at the 17th parallel north area, the view of the Earth is seen at the lunar sky all year round at around 73 degrees facing south and at about 31 degrees towards the west from the top.
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