Jump to content

Dorsum Cayeux

From Wikipedia, the free encyclopedia

This is the current revision of this page, as edited by Finlay McWalter (talk | contribs) at 08:44, 4 June 2019 (WP:SECTIONORDER, MOS:HEAD, ce). The present address (URL) is a permanent link to this version.

(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)
Oblique view from Apollo 11, with Taruntius P and K in lower left

Dorsum Cayeux is a wrinkle ridge at 1°36′N 51°12′E / 1.6°N 51.2°E / 1.6; 51.2 in Mare Fecunditatis on the Moon. It is approximately 95 km long and was named after French geologist Lucien Cayeux in 1976 by the IAU.[1]

Dorsum Cayeux begins on the north side of Taruntius P crater and trends to the northwest past Taruntius K crater, and then it curves back to the northeast and flattens out into the mare surface northwest of Smithson crater. The ridge is probably a continuation of Dorsa Geikie, which ends on the south side of Taruntius P crater (i.e., the object that created Taruntius P impacted the ridge).

References

[edit]
  1. ^ Dorsum Cayeux, Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN)
[edit]