The basin containing Mare Nubium is believed to have been part of the Pre-Nectarian system. The mare material is of the Imbrian and Eratosthenian age.
Bullialdus crater, a prominent feature on the west side of the mare, is of Eratosthenian age. Other features within the mare include Pitatus on the southern margin and Guericke bounding the mare to the north. Opelt, Gould, Kies, Nicollet, Wolf, Birt, and Rupes Recta (the Straight Wall) lie within the mare.
Like most of the other maria on the Moon, Mare Nubium was named by Giovanni Riccioli, whose 1651 nomenclature system has become standardized. Previously, William Gilbert had included it among the Continens Meridionalis ("Southern Continent") in his map of c.1600, and Michael Van Langren had labelled it the Mare Borbonicum (after the House of Bourbon) in his 1645 map.
The first released images from the Lunar Reconnaissance Orbiter in 2009 were of the lunar highlands 200 km south of Mare Nubium.
In September 2013, Spanish astronomers observed and recorded an impact event when a large rock hit the lunar surface in Mare Nubium.
- ^ "Mare Nubium". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
- ^ "Mare Nubium". NASA Lunar Atlas. Archived from the original on 2009-06-04. Retrieved 2009-07-04.
- ^ "Impact Basin Database". Archived from the original on 2014-08-07. Retrieved 2017-01-23.
- ^ Geologic Map of the Near Side of the Moon, USGS I-703, Don E. Wilhelms and John F. McCauley, 1971 (L&PI web version)
- ^ "Observatorio ARVAL - Moon Map". Observatorio ARVAL. Retrieved 2009-07-04.
- ^ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.61.
- ^ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.15
- ^ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.41, 198.
Garner, Robert (July 2, 2009). "LRO's First Moon Images". NASA. Retrieved February 16, 2015.
- ^ "Astronomers spot record-breaking lunar impact". Phys.Org. Retrieved 2014-02-25.