Craterra

Northern Mare Tranquillitatis

A Late Imbrian Landmark on the Edge of Mare Tranquillitatis

Sitting along the northern edge of Mare Tranquillitatis, Vitruvius displays an uneven rim, a dark interior floor, and proximity to the Apollo 17 landing site.

Feature Profile & Selenographic Data

Feature type
crater
Coordinates
17.66° N · 31.28° E
Diameter
30.94 km
IAU approval
1935/01/01 00:00:00
LAC quadrangle
LAC-43 · Macrobius
Geological Period
Late Imbrian

Geological Chronicle

Vitruvius is a lunar impact crater measuring 30.94 kilometers in diameter on the northern edge of Mare Tranquillitatis. Gardner lies to the east, Fabbroni to the northeast, and the elongated mountain Mons Vitruvius rises to the north-northwest, beyond which lies the valley where the Apollo 17 mission landed.

On the lunar geologic timescale, Vitruvius dates to the Late Imbrian age. T. W. Webb recorded that Vitruvius has a very dark interior. The interior floor is uneven, with low rises in the southwest, and a small crater is attached to the southern outer rim.

The rim of Vitruvius is somewhat circular, but its sides are uneven to the north and east, rising highest to the northwest. The landmark was named after Marcus Vitruvius Pollio, the ancient Roman engineer and architect.

Scientific Sources & References

Name Origin

Vitruvius Pollio, Marcus; Roman engineer, architect (unkn-fl. c. 25 B.C.).

Interactive Lunar Surface

Explore Vitruvius in 3D

Inspect lunar elevation data and the official selenographic position.