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File:Mare Orientale - C.jpg

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English: en:Mare Orientale straddles both the near and far side. The basin has the most nearly complete concentric ring structure of any basin in the west. The surrounding basin material is of the Lower Imbrian epoch, with the mare material being of the Upper Imbrian epoch. The outermost conspicuous ring is Cordillera, bounded inwardly by steep scarp or gentle lip and topped by some ridgelike massifs. The mare-like material to the northeast is Lacus Autumni. You can also make out the crater Maunder among the northern region of the mare. Off to the southeast of Maunder is Kopff. Montes Rooks lines the eastern edge of the mare.
Source http://lunar.arc.nasa.gov/science/atlas/mare/morientale.htm (https://web.archive.org/web/20130221171721/http://lunar.arc.nasa.gov/science/atlas/mare/morientale.htm)
Author NASA


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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current01:07, 1 June 2007Thumbnail for version as of 01:07, 1 June 2007350 × 382 (20 KB)Bryan Derksen (talk | contribs){{Information |Description={{en|en:Mare Orientale straddles both the near and far side. The basin has the most nearly complete concentric ring structure of any basin in the west.The surrounding basin material is of the Lower Imbrian epoch, with the

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