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.
Right now scientists do not know why the Earth-facing side of the moon has thicker crust. One proposal is that Earth may have once had two moons that collided at relatively low speeds. The geologically different regions on the moon would then have originated from two separate moons.
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.