Mare Nubium
Contents
Nubium Basin
(unofficial name; IAU feature name for central 715 km of mare: Mare Nubium)
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Lat: 21.3°S, Long: 16.6°W, Main ring diam: 690 km, Basin depth: 1.63 km, Rükl: 54 |
Left: Howard Eskildsen, Right: Clementine, Clementine LIDAR Altimeter texture from PDS Map-a-Planet remapped to north-up aerial view by LTVT. The dot is the center position and the white circle the main ring position from Chuck Wood's Impact Basin Database. Grid spacing = 10 degrees.
Table of Contents
[#Nubium Basin Nubium Basin]
[#Nubium Basin-Images Images]
[#Nubium Basin-Maps Maps]
[#Nubium Basin-Basin Classification Basin Classification]
[#Nubium Basin-Description Description]
[#Nubium Basin-Description: Wikipedia Description: Wikipedia]
[#Nubium Basin-Additional Information Additional Information]
[#Nubium Basin-Nomenclature Nomenclature]
[#Nubium Basin-LPOD Articles LPOD Articles]
[#Nubium Basin-Bibliography Bibliography]
Images
LPOD Photo Gallery Lunar Orbiter Images Apollo Images
WARNING: the LPI's list of orbital Apollo photographs of Mare Nubium shows a series of Apollo 17 photographs. Impossible because Apollo 17's belt of orbits was way too north to make detailed photographs of Mare Nubium! (which was behind or very near the curved southern horizon).- DannyCaes DannyCaes Jul 30, 2010
Maps
(LAC zone 94B4) LAC map Geologic map
Basin Classification
(description of terms and most numeric basin data from Wood, C.A. (2004) Impact Basin Database)
| Certainty of Existence |
USGS Age |
Wilhelms Age Group |
Ring Diameters |
Mare Thickness |
Mascon |
| Uncertain |
Pre-Nectarian |
3 |
690 km |
Description
The pre-Nectarian Mare Nubium covers geographically nearly two-thirds of the area under study, centred at 21.3 S 16.6 W. Its official name since 1935, Mare Nubium, or “Sea of Clouds”, derives from early telescopic observations. The mare’s numerous ghost features, and various higher-albedo crater ejecta criss-crossing the basin, conjured up the idea of lunar clouds.
Mare Nubium has a diameter of 750 km, and it is one of the most ancient circular basins on the Moon (Stuart-Alexander and Howard, 1970). Nevertheless, there is clear evidence that the basin did not form by a single large impact. Its present morphology appears to be a consequence of a number of major collisions. Morphological evidence of at least four major basin rings is still clearly identifiable (i.e. De Hon, 1977).
Description: Wikipedia
Additional Information
On September the 11th of 2013, a bright impact flash was observed at Mare Nubium. See LPOD Forming a New Crater.
Nomenclature
The IAU feature name means "Sea of Clouds".
- Named Continens Meridionalis (Southern Continent) in pre-telescopic sketch map by William Gilbert in ~1600. Name also included Cognitum, Insular and Humorum! [Whitaker: Mapping and Naming the Moon, p 15]
- The impact basin is named after the mare.
LPOD Articles
Forming a New Crater (the bright impact flash of September the 11th, 2013)
Bibliography
Stratigraphy and composition of lava flows in Mare Nubium and Mare Cognitum
This page has been edited 1 times. The last modification was made by - tychocrater tychocrater on Jun 13, 2009 3:24 pm - afx3u2
