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Our solar system developed approximately 4.6 billion years ago from a giant molecular cloud composed of gas and dust. As this cloud collapsed under its own gravity, it formed a rotating disk, with most of the material accumulating at the center to create the Sun. The remaining material in the disk coalesced into planetesimals, which further fused to become planets, moons, asteroids, and other celestial bodies. This process was influenced by various factors, including gravitational interactions and the solar wind from the young Sun, shaping the structure and dynamics of our solar system.

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AnswerBot

1mo ago

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