The Origin of the Moon
Moon rocks hold important clues to the origin of the satellite. The results of analyzing these Moon rocks have led scientists to conjecture that the Moon may have formed 4.5 billion years ago when the Earth collided with a very large object (the size of Mars or larger), ejecting raw materials that eventually became the Moon. This is known as the impact theory. Currently, the impact theory is conceivably the one most widely accepted by scientists, but other theories do exist and have significant support.
Coaccretion theory holds that the Moon formed in Earth's orbit along with all the other planets in the Solar System, so that there were two planets in the same orbit for some time before the moon was taken over by the earth's gravity.
Fission theory states that, when the Solar System was very young, the Earth was spinning so fast (nearly 10,000 miles per hour (16,000 km/hr), or ten times its current speed), that it threw off a large chunk of material in order to stabilize itself and slow down; that chunk, the theory holds, became the Moon.
Capture theory holds that the Moon was formed elsewhere in the Solar System and was seized by the Earth.
Of all these theories, the impact theory fits best with all the data that has thus far been accumulated about the Moon. Future lunar exploration, such as the determination of the bulk composition of the Moon, should help scientists settle this issue.
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