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The formation of the solar system was primarily influenced by the gravitational collapse of a giant molecular cloud, known as the solar nebula, approximately 4.6 billion years ago. As the nebula collapsed, it spun and flattened into a disk, where the Sun formed at the center while the remaining material coalesced into planets, moons, asteroids, and comets. Key factors include the conservation of angular momentum, temperature gradients within the disk, and the processes of accretion and differentiation. Additionally, interactions with nearby stars and supernovae may have played a role in triggering the collapse of the solar nebula.

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3mo ago

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