Craterra

Mare Fecunditatis Wrinkle Ridge

Dorsa Mawson

A 143-kilometer wrinkle ridge system in Mare Fecunditatis named after Antarctic explorer Douglas Mawson.

Feature Profile & Selenographic Data

Feature type
dorsum
Coordinates
7.77° S · 52.48° E
Diameter
142.71 km
IAU approval
1979/01/01 00:00:00
LAC quadrangle
LAC-80 · Langrenus

Geological Chronicle

Dorsa Mawson is a wrinkle ridge system located in Mare Fecunditatis on the Moon. The feature extends across the region for an official length of 142.71 kilometers.

The southern end of the ridge is located near Crozier M crater, southeast of ibn Battuta crater, and trends roughly northeast toward unnamed craters between Lindbergh and Bilharz craters. The International Astronomical Union officially named the ridge system in 1979 after Antarctic explorer Douglas Mawson.

Chronology & Exploration

  1. 1979 IAU Name Adoption

    The International Astronomical Union officially named the wrinkle ridge system after Antarctic explorer Douglas Mawson.

Scientific Sources & References

Name Origin

Douglas; English-Australian Antarctic explorer (1882-1958).

Interactive Lunar Surface

Explore Dorsa Mawson in 3D

Inspect lunar elevation data and the official selenographic position.