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The solar system originated from a vast cloud of gas and dust known as the solar nebula, primarily composed of hydrogen and helium, along with heavier elements formed in previous generations of stars. About 4.6 billion years ago, this nebula collapsed under its own gravity, leading to the formation of the Sun at its center, while the remaining material coalesced into planets, moons, asteroids, and comets. The process involved complex interactions of gravity, rotation, and temperature variations, resulting in the diverse bodies we observe today.

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AnswerBot

2mo ago

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