During the early stages of the Earth and Moon (relatively early) the Earth was very hot. The Moon was much closer to Earth at that time, and the heat from the Earth made material transfer to the far side of the Moon. This resulted in a thicker crust. When the Earth and Moon were hit by many asteroids, magma from the inner Moon oozed out onto the surface and cooled in to Maria. But on the far side, the crust was thicker so not as many collisions could penetrate the surface, resulting in fewer maria.
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B: The Phases of the Moon.
All sides are lit up. Only one side at a time. There is a term called the dark side of the moon. This term relates to the fact that the moon doesnt spin on its axis like the earth does and one side faces the earth all of the time. The dark side refers not to the abscence of light but radio waves. During the Apollo missions to the moon, as a spacecraft went behind the moon (in relation to the earth) It went into whats called a radio blackout. It was called the dark side because up until the first spacecraft orbited the moon, it had never been seen by man before.
During the New moon, the lighted side of the Moon is the OTHER side, the side we never see.
It is weaker
Low altitude areas on the moon are called maria, which are large dark plains formed by ancient volcanic activity. The maria are located on the side of the moon that faces Earth.
The maria on the Moon are large, dark, flat plains formed by ancient volcanic activity, while the highlands are rugged, elevated regions composed of older, lighter-colored rocks. The maria are mainly on the side of the Moon facing Earth, while the highlands are more prevalent on the far side. These varying terrains give the Moon its distinctive appearance when viewed from Earth.
The feature that covers much of the Moon's surface is called the maria, which are large, dark, basaltic plains formed by ancient volcanic eruptions. The maria are mainly located on the side of the Moon facing Earth.
more maria.
Lunar Maria-'Maria' is a Latin word meaning "seas". The singular form is mare. They are large, dark, balsaltic plains found on the surface of the moon. Astronomers believe they were originally formed by ancient volcanic eruptions. To the naked eye, they appear very dark, and this is due to iron-rich composition. They cover nearly 15% of the moon's surface - most of which is on the near side to the Earth (the side we can see).In fact, it is because of Lunar Maria that people often think they see a face in the moon.
The large dark flat areas on the Moon, known as "maria" (singular: "mare"), are vast basaltic plains formed by ancient volcanic eruptions. They are primarily located on the side of the Moon that faces Earth, while the far side, which also has maria, appears more rugged and heavily cratered. The far side's maria are less visible from Earth due to the Moon's synchronous rotation, which keeps one hemisphere facing us at all times. As a result, features on the far side remain largely unexplored and unseen by the naked eye from our planet.
The far side of the Moon has more craters because it lacks the large expanses of dark, smooth volcanic maria that are present on the near side. These maria shielded the near side from impacts, preserving its surface. Additionally, the far side is more exposed to incoming asteroids and meteoroids due to its position away from Earth, leading to more frequent impacts.
The moon appears smooth on one side, known as the near side, because it is covered by large, flat plains called maria, formed by ancient volcanic activity. In contrast, the far side is heavily cratered and rugged, with fewer maria, due to its thicker crust and less volcanic activity. This difference is a result of tidal locking, where the same side of the moon always faces Earth, allowing for varied geological processes on each side.
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Phases of the moon.
Almost all the maria are on the near side. The far side is mostly just craters.
phases of the moon.