Da Vinci (lunar crater)
Lunar crater
From Wikipedia, the free encyclopedia
da Vinci is a degraded lunar impact crater that is located in the eastern part of the Moon, to the northwest of Mare Fecunditatis.[2] It lies along the eastern shore of the Sinus Concordiae, a bay along the eastern edge of Mare Tranquillitatis. Nearby craters include Watts to the southeast and Lawrence to the southwest, both smaller in dimension than da Vinci.[3]
Lunar Orbiter 4 image | |
| Coordinates | 9.1°N 45.0°E |
|---|---|
| Diameter | 37.46 km (23.28 mi)[1] |
| Depth | Unknown |
| Colongitude | 316° at sunrise |
| Eponym | Leonardo da Vinci |

This formation has been heavily damaged and reshaped until it is scarcely recognizable as a crater. Sections of the low eastern rim and a portion to the northwest are still somewhat intact, although they more closely resemble curved ridges than a crater wall. There are gaps in the rim to the south and north, and the interior is irregular with portions having been resurfaced.[4]: 61
The terrain along the northern and western exterior of the crater is irregular and hilly. A low ridge to the southeast runs to the vicinity of Watts.
This formation is named after the Italian artist, inventor, and mathematician, Leonardo da Vinci (1452-1519).[1] His name was introduced into lunar nomenclature by the Austrian geographer Karl Peucker.[5] Its designation was officially adopted by the International Astronomical Union in 1935.[1]
Satellite craters
See also
- 3000 Leonardo (asteroid named for Leonardo da Vinci)