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When the solar system was first forming, about 4.6 billion years ago, it began as a vast cloud of gas and dust known as the solar nebula. This nebula collapsed under its own gravity, leading to the formation of the Sun at its center, while the remaining material started to coalesce into planets, moons, and other celestial bodies through processes like accretion and differentiation. As the planets formed, they experienced significant heating, leading to differentiation into layers based on density. This period was marked by intense activity, including collisions and the clearing of debris, ultimately shaping the solar system we observe today.

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1d ago

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