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  • Also known as Rima Hadley, this [[rille]] is located within Mare Imbrium and is near the location of the [[Apollo 15]] moon landing in an area calle
    1 KB (227 words) - 18:13, 10 August 2008
  • ...n in this image, which is reddish to the southeast, dominated by excavated mare lava, and bluish to the northwest, caused by the excavation of highland mat
    3 KB (488 words) - 23:42, 16 October 2008
  • ...eform the lunar surface. Examples of these forces include the formation of mare ridges and arcuate rilles, along with relatively weak moonquakes. The force ...telescopes, around the lunar basins. A particularly stunning set occurs on Mare Humorum.
    10 KB (1,630 words) - 03:36, 29 October 2008
  • This is a list of ''[[lunar mare|maria]]'' (singular ''mare'') on the [[Moon]]. | [[Mare Anguis]]
    10 KB (1,414 words) - 23:38, 1 February 2011
  • ...ng for geologic concentrations of KREEP-bearing materials. The rim of Mare Imbrium is neatly traced by thorium's gamma ray emissions as detected by [[Lunar Pr
    20 KB (374 words) - 03:31, 3 October 2009
  • ...P is mainly concentrated in the area of [[Oceanus Procellarum]] and [[Mare Imbrium]]. This unusual geological region is now referred to as the [[Procellarum ...samples are believed to have originated after the impact which formed the Imbrium basin[http://www.nature.com/nature/journal/v336/n6201/abs/336751a0.html].
    6 KB (854 words) - 20:19, 18 June 2015
  • ...arded $97 million and has proposed to fly as many as four payloads to Mare Imbrium, a lava plain in one of the Moon’s craters, by September 2020." <ref name
    5 KB (779 words) - 18:38, 23 June 2019
  • ...s concentrated in the [[Oceanus Procellarum]] (Ocean of Storms) and [[Mare Imbrium]] (Sea of Rains) with a major concentration south of [[Crater Copernicus]].
    7 KB (1,101 words) - 09:57, 27 April 2013
  • #[http://lroc.sese.asu.edu/posts/5 Apollo Basin: Mare in the Sea of Highlands] #[http://lroc.sese.asu.edu/posts/6 Chain of Secondary Craters in Mare Orientale]
    53 KB (7,303 words) - 06:50, 13 July 2019
  • ...ejecta forms a ‘hummocky’ terrain (examples of this can be seen around the Imbrium basin as the Fra Maruo formation, and around the Nectaris Basin as the Jans ...er 15 meters thick on the lunar highlands, and up to 8 meters thick on the mare. Because the regolith is so thick, it acts as a protective shield to the
    21 KB (3,529 words) - 17:17, 3 August 2013