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How the Solar System Formed
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About 4.6 billion years ago an interstellar cloud of gas and dust began to collapse under the force of its own gravity.
As the cloud collapsed, it began to rotate and flatten into a spinning disk. The large clump of gas at the center became the Sun.
Gas and dust around the newborn Sun began to clump into larger objects. The surfaces of early planets were bombarded by comets and asteroids left over from the original disk.
The bombardment gradually declined during the first half-billion years, but the comets and asteroids remaining still occasionally collide with planets — sometimes with dramatic consequences.
 

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