Attēls:Mare Anguis.jpg

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Mare_Anguis.jpg(350 × 382 pikseļi, faila izmērs: 19 KB, MIME tips: image/jpeg)

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English: en:Mare Anguis is in the middle of the picture. It is located on the near side of the moon (the side facing the Earth), and is about 150 miles in diameter. Located within the Crisium basin, Mare Anguis is a part of the Nectarian System, meaning that it was formed during the Nectarian time period (according to Wilhelms, 1987 (Plate 9A) - Upper Imbrian epoch). Like most maria, the surface of Mare Anguis is dark, indicating that it has been filled with volcanic basalt. The crater at the left center is Eimmart, at the northwestern tip of Mare Anguis. The dark patch in the lower left corner is the northeastern edge of Mare Crisium.
Avots http://lunar.arc.nasa.gov/science/atlas/mare/manguis.htm (archive)
Autors 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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tagadējais2007. gada 1. jūnijs, plkst. 03.492007. gada 1. jūnijs, plkst. 03.49 versijas sīktēls350 × 382 (19 KB)Bryan Derksen{{Information |Description={{en|en:Mare Anguis is seen in the middle of the picture below. It is located on the near side of the moon (the side facing the Earth), and is about 150 miles in diameter. Located within the Crisium basin, Mare Anguis is a

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