Meteorites can make large depressions on Earth’s surface when they make impact. Why are so few of these depressions visible on Earth’s surface?

• Earth is constantly changing it’s topography due to volcanic activity, or processes such as weathering, erosion, and deposition. ***
• Since Earth’s surface is mostly water, it is difficult for a meteorite to make a depression that can be seen.
• The meteorite became buried underground so the actual depression is filled by the meteorite.

The correct answer is:

• Earth is constantly changing its topography due to volcanic activity or processes such as weathering, erosion, and deposition.

The correct answer is: Earth is constantly changing its topography due to volcanic activity, or processes such as weathering, erosion, and deposition.

The reason why so few meteorite impact craters are visible on Earth's surface is because our planet undergoes continuous geological processes that constantly reshape its topography. Volcanic activity, for example, creates new landforms and can bury or erase existing craters. In addition, processes such as weathering, erosion, and deposition also contribute to the gradual transformation of the Earth's surface.

Over time, weathering breaks down rocks and other geological features, while erosion carries away the particles and sediments. This can blur or erase the evidence of past meteorite impacts. Furthermore, deposition occurs when sediments are laid down in new areas, potentially burying any visible depressions created by meteorites.

It is important to note that while a small number of meteorite impact craters have been identified on Earth's surface, many more are believed to exist but are not immediately visible due to these constantly changing geological processes.

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