Craterra

Mare Serenitatis

A Wrinkle Ridge Traversing Mare Serenitatis

Located in Mare Serenitatis, this 183-kilometer wrinkle ridge trends from south to north along approximately the lunar 12th parallel.

Feature Profile & Selenographic Data

Feature type
dorsum
Coordinates
23.60° N · 11.95° E
Diameter
183.06 km
IAU approval
1976/01/01 00:00:00
LAC quadrangle
LAC-42 · Mare Serenitatis

Geological Chronicle

Dorsum Von Cotta is a wrinkle ridge located within Mare Serenitatis on the Moon. Extending 183 kilometers, the feature trends south to north at approximately the lunar 12th parallel.

Hornsby crater is located to the east of the ridge, while the collapse feature Aratus CA lies to the west. To the south is Dorsum Buckland.

The ridge was officially named in 1976 in honor of German geologist Bernhard von Cotta.

Chronology & Exploration

  1. 1976 Official Designation

    The International Astronomical Union officially named the ridge after German geologist Bernhard von Cotta.

Scientific Sources & References

Name Origin

Carl Bernard; German Earth scientist (1808-1879).

Interactive Lunar Surface

Explore Dorsum Von Cotta in 3D

Inspect lunar elevation data and the official selenographic position.