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Lunar mare are dark, smooth plains formed by ancient volcanic activity, while lunar highlands are lighter-colored, rugged terrains composed of mountains, hills, and craters. Mare regions have fewer impact craters than highlands, indicating younger geological features. Mare plains formed from lava flows that filled large impact basins, while highlands represent the original lunar crust.
Dark places on the moon are called lunar maria, which are large, flat, dark-colored basaltic plains formed by ancient volcanic activity. These areas contrast with the brighter highlands on the moon's surface.
A dark area on the Moon, known as a lunar mare, is a large basaltic plain formed by ancient volcanic activity rather than water. These areas appear darker than the surrounding highlands due to their lower reflectivity of sunlight.
The feature covering much of the moon's surface is the lunar mare, which are large dark plains formed by ancient volcanic activity. These mare areas are less cratered compared to the highlands and are thought to be composed of basalt rock.
The dark spots on the moon are called lunar maria, which are large plains formed by ancient volcanic activity. The lighter areas are called highlands, which are rugged and densely cratered regions of the moon's surface.
Mare Tranquillitatis or Sea of Tranquility is the lunar landform.
Some landed in the Mare, some landed in the highlands.
Lunar features often refer to various geological formations found on the Moon's surface, including maria (large, dark basaltic plains), highlands (lighter, rugged areas), craters (impact sites), and rilles (channel-like structures). Commonly discussed pairs include the large maria, such as Mare Imbrium and Mare Serenitatis, and prominent craters like Tycho and Copernicus. Additionally, the contrast between the smooth, flat maria and the mountainous highlands exemplifies the Moon's diverse geological landscape. These features provide insights into the Moon's history and the processes that shaped it.
The broad flat lava plains on the moon are known as maria, which is Latin for seas. These plains were formed by extensive volcanic activity billions of years ago, and they appear dark due to their low reflectivity compared to the surrounding highlands. The most famous example of a lunar mare is the Sea of Tranquility, where the Apollo 11 mission landed in 1969.
Mare Tranquillitatis (Latin for Sea of Tranquility) is a lunar mare that sits within the Tranquillitatis basin on the moon.
the two sides on the moon are highland and the mare. the mare are lower in altitude than the highlands . but there is no water on the moon so they are not literally seas .
Mares: Are fully grown filly's or adult female horses.Mare: Latin word for "sea".Mare: Used when describing the flat plains on the moon - as in Lunar Mare. A basaltic plain on the Moon