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File:Mare Anguis.jpg

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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.
来源 http://lunar.arc.nasa.gov/science/atlas/mare/manguis.htm (archive)
作者 NASA


Public domain 本文件完全由NASA创作,在美国属于公有领域。根据NASA的版权方针,NASA的材料除非另有声明否则不受版权保护。(参见Template:PD-USGov/zhNASA版权方针页面JPL图片使用方针。)
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当前2007年6月1日 (五) 00:492007年6月1日 (五) 00:49版本的缩略图350 × 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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