There can be craters anywhere on the moon, not just the side we see
Two types of moon craters are impact craters, formed by asteroids or meteoroids hitting the moon's surface, and volcanic craters, formed by volcanic activity on the moon when magma rises to the surface and erupts.
The two sides of the moon are the near side and the far side. The near side is the side facing Earth and is more flat with dark areas called maria. The far side is more rugged with highlands and fewer maria.
The two sides of the moon, known as the near side and the far side, have distinct differences. The near side of the moon is the side that faces Earth and is more flat and smooth with large dark areas called maria. The far side of the moon is more rugged and mountainous with fewer maria. Additionally, the far side has a thicker crust and is not visible from Earth due to synchronous rotation.
The Moon spins at the same rate that it orbits the Earth, keeping one face turned toward the Earth. The terms "near side" and "far side" are correct to describe the two sides of the Moon. Until the Soviet Luna 3 satellite orbited the Moon in 1959, we had no clue what the far side of the Moon looked like.
Craters on the moon were formed primarily through two processes: impact from meteoroids and volcanic activity. Impact craters were created when meteoroids collided with the moon's surface, causing large depressions. Volcanic craters, on the other hand, formed when volcanic activity released magma and gases, creating bowl-shaped depressions.
Two types of moon craters are impact craters, formed by asteroids or meteoroids hitting the moon's surface, and volcanic craters, formed by volcanic activity on the moon when magma rises to the surface and erupts.
The two sides of the moon are the near side and the far side. The near side is the side facing Earth and is more flat with dark areas called maria. The far side is more rugged with highlands and fewer maria.
meteors and asteroid fragments.
The two sides of the moon, known as the near side and the far side, have distinct differences. The near side of the moon is the side that faces Earth and is more flat and smooth with large dark areas called maria. The far side of the moon is more rugged and mountainous with fewer maria. Additionally, the far side has a thicker crust and is not visible from Earth due to synchronous rotation.
The Moon spins at the same rate that it orbits the Earth, keeping one face turned toward the Earth. The terms "near side" and "far side" are correct to describe the two sides of the Moon. Until the Soviet Luna 3 satellite orbited the Moon in 1959, we had no clue what the far side of the Moon looked like.
He found that the Earth moves around that sun. The surface of the moon seemed pitted with craters. and the third one I don't know. Hope the other two help! :)
Craters on the moon were formed primarily through two processes: impact from meteoroids and volcanic activity. Impact craters were created when meteoroids collided with the moon's surface, causing large depressions. Volcanic craters, on the other hand, formed when volcanic activity released magma and gases, creating bowl-shaped depressions.
Earth is biologically active. Life - mainly vegetative - keeps filling the craters in. Edit: in fact these are the main reasons, as far as I know : 1) Erosion caused by weather 2) Concealment by sediments 3) Renewal of the Earth's surface by tectonic plates.
The most heavily cratered object in the solar system is thought to be Callisto, the second-largest moon of Jupiter.This does not necessarily indicate that it has been more heavily bombarded than other bodies (for example, the "far side" of the Moon, which is hit by bodies drawn toward Earth). It only means that the craters have not been eroded or erased by the exterior processes of the planet or Moon.As far as total impacts, the planet Mercury has slightly greater area than Callisto, and substantial cratering. The largest moon of Jupiter, Ganymede, also has its fair share despite tectonic smoothing.
It reflects light from the Sun and it has different phases.
The largest crater on the moon is the Aitken Basin. It is 2500 km in diameter and 13km deep. It is located near the Lunar south pole and is not viable from Earth. It is thought to be one of the largest craters in the solar system.Hertzprung is the second largest crater on the moon. It is 591 km in diameter and it located on the dark side of the moon just beyond the west limb.Apollo Crater is the third largest crater on the moon. It is located near the south pole on the far side of the moon. it is 538 km in diameter but its depth is unknown.Korolov Crater is about 437 km in diameter and is located close to the lunar equator on the far side of the moon.Bailly crater is the largest crater visible from Earth. It is 303 km in diameter and 4.3 km deep. Located near the south west limb of the moon.Some craters have flooded with molton lava after the impact. They are now called mare or seas.Mare Ibrium at 1,123 km in diameter is the largest.Mare Tranquillitatis made famous by the Apollo 11 moon landing, is about 873km in diameter.Mare Nubium is about 715 km in diameter.Apollo 17 landed near Mare Serenitatis. It is 707 km in diameter.Mare Orientale is about 327 km in diameter.
The word crater (meaning bowl-shaped) is applied to two different phenomena.On planets and moons, meteor craters are the circular depressions caused by the impacts of other objects, mainly smaller asteroids and meteoroids. They are prominent on the Moon and on the planet Mercury. Some objects hit Earth in the past, but only a few landmarks still exhibit their characteristic bowl shape.The other use is to describe a volcanic caldera, or inner depression within a volcano. Many dormant volcanoes have solidified craters in their peaks, some with lakes or glaciers.