Fichier:Mare Marginis.jpg

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English: en:Mare Marginis lies on the very edge of the lunar nearside. It differs from most of the nearside maria. It has an irregular outline, and it appears to be fairly thin. Note the small circular and elongated features in the mare plains. These probably mark impact craters buried by less than 1000 - 1700 feet of lava. Further, Mare Marginis is not centered on any clear, large impact basin. Thus, Mare Marginis seems to mark a low-lying region of the highlands where mare lavas were just able to reach the surface. Several large mare-floored craters also occur nearby. In these craters, the crater floors lie below the surrounding highland surface. Thus, they mark sites around Mare Marginis where lavas were close to the lunar surface. The major crater to the north of Marginis Al-Biruni, with Ibn Yunus to the southeast, and Goddard to the northwest.
Quell http://lunar.arc.nasa.gov/science/atlas/mare/mmarginis.htm
Auteur NASA
Public domain Diese Datei ist gemeinfrei (public domain), da sie von der NASA erstellt worden ist. Die NASA-Urheberrechtsrichtlinie besagt, dass „NASA-Material nicht durch Urheberrecht geschützt ist, wenn es nicht anders angegeben ist“. (NASA-Urheberrechtsrichtlinie-Seite oder JPL Image Use Policy).
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aktuell06:02, 31. Mee 2007Miniaturbild fir d'Versioun vum 06:02, 31. Mee 2007350 × 382 (12 KB)Bryan Derksen{{Information |Description={{en|en:Mare Marginis lies on the very edge of the lunar nearside. It differs from most of the nearside maria. It has an irregular outline, and it appears to be fairly thin. Note the small circular and elongated features in

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