small meteorite impacts, gravity pulling sediment down slopes, weathering of rock and sediment due to temperature changes from day to night
Earth's shadow on the moon proved that earth wasn't flat. When galileo first turned his telescope to the moon, he found a surface scarred by craters and maria. Before that time, many people believed that all planetary bodies were "perfect" without surface features.
Earth's moon (surface area) - 14,645,750 square miles.
New moon.
The surface of the moon heats up.
Neptune's moon has significant information when observing its surface features, composition, and interactions with Neptune's magnetosphere. Data collected from flybys and orbital missions provide valuable insights into the moon's geology, atmosphere, and history, shedding light on its formation and evolution within the Neptune system.
Space particles, such as meteoroids, are able to bombard the Moon's surface because the Moon lacks a thick atmosphere to burn up or slow down these particles. As a result, meteoroids collide with the Moon's surface at high velocities, creating impact craters and shaping its landscape over time. These impacts contribute to the ongoing geological evolution of the Moon.
The size of the object crashing into the lunar surface. There is no atmosphere on the moon to slow down approaching objects (as there is on Earth). This means that chunks of space 'rock' don't disintegrate on their way to the moon's surface.
Slow Dancing with the Moon was created in 1992.
The outer surface of the moon is called the crust.
It means our centre or bass of evolution.
The surface features and distribution on the Moon's surface provide clues about its geological history, including impact cratering, volcanic activity, and tectonic processes. By studying these features, scientists can infer the sequence of events that shaped the Moon over time, such as the formation of large impact basins and the eruption of lava flows. This information helps us understand the Moon's formation and evolution.
The surface features on the Moon, like cracks, are often the result of various geological processes, such as impacts from meteoroids or volcanic activity. Over time, these cracks may widen or close due to additional impacts or the Moon's own gravitational forces. Studying such features can provide valuable insights into the Moon's history and its geological evolution.
The moon's surface is regolith (ground up rock).
The moon has a solid (terrestrial) surface.
The moon does have gravity, just less than Earth's. When a rocket lands on the moon, it is pulled towards the moon's surface by its gravity, similar to how objects are pulled towards Earth. The rocket's engines are used to slow down its descent and land safely on the moon's surface.
The slow rotation of the moon means that each lunar day and night lasts about 14 Earth days. This leads to extreme temperature differences with surface temperatures reaching over 200 degrees Fahrenheit during the day and dropping to well below freezing at night. The lack of atmosphere on the moon also means that there is no way to trap heat, further contributing to these temperature extremes.
Earth's shadow on the moon proved that earth wasn't flat. When galileo first turned his telescope to the moon, he found a surface scarred by craters and maria. Before that time, many people believed that all planetary bodies were "perfect" without surface features.