|Diameter||715 km (444 mi)|
|Eponym||Sea of Clouds|
The basin containing Mare Nubium is believed to have been part of the Pre-Nectarian system, with the surrounding basin material being of the Lower Imbrian epoch. The mare material is of the Upper Imbrian epoch.
The crater to the west of the mare is Bullialdus, which is of the Eratosthenian Epoch. This means the crater is younger than the mare it sits in. The crater that sits on the southern rim of the mare is Pitatus.
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.
In September of 2013, Spanish astronomers observed and recorded an impact event when a large rock hit the lunar surface in Mare Nubium
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- "Mare Nubium". NASA Lunar Atlas. Retrieved 2009-07-04.
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- 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.