File:Mare Serenitatis - Clementine.jpg

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Mare_Serenitatis_-_Clementine.jpg ‎(350 × 382 pixels, file size: 34 KB, MIME type: image/jpeg)

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English: Mare Serenitatis sits just to the east of Mare Imbrium. It is located within the Serenitatis basin, which is of the Nectarian epoch. The material surrounding the mare is of the Lower Imbrian epoch, while the mare material is of the Upper Imbrian epoch. The mare basalt covers a majority of the basin and overflows into Lacus Somniorum to the northeast. The most noticeable feature is the crater Posidonius on the northeast rim of the mare. The ring feature to the west of the mare is indistinct, except for Montes Haemus. Mare Serenitatis connects with Mare Tranquillitatis to the southeast.
Source http://lunar.arc.nasa.gov/science/atlas/mare/mserenitatis.htm (archive)
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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current01:42, 30 August 2014Thumbnail for version as of 01:42, 30 August 2014350 × 382 (34 KB)Sneeuwschaap (talk | contribs)+brightness
01:09, 1 June 2007Thumbnail for version as of 01:09, 1 June 2007350 × 382 (16 KB)Bryan Derksen (talk | contribs){{Information |Description={{en|en:Mare Serenitatis sits just to the east of Mare Imbrium . it is located within the Serenitatis basin, which is of the Nectarian epoch. The material surrounding the mare is of the Lower Imbrian epoch, while themare ma

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