Mare Marginis

Mare Marginis

Mare Marginis (łac. Morze Brzegowe) to morze księżycowe położone zarówno po widocznej, jak i po niewidocznej stronie Księżyca. Jego średnica równa jest 420 km.

Współrzędne selenograficzne: 13,3° N, 86,1° E.

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Full Moon Luc Viatour.jpg
(c) Luc Viatour, CC-BY-SA-3.0
Nearly Full Moon view from earth In Belgium (Hamois).
Mare Marginis.jpg
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.