Formation of Solar System Summary

Definition

The process of the Solar System's creation, where planets, asteroids, and comets formed from a flat disk of material around the Sun. Inner planets were warmer, smaller, and rocky, while outer planets were colder and larger, with ice mixed in. Gravity from outer planets influenced the movement of ice chunks, leading to the formation and distribution of comets.

Summary

The formation of the solar system is a complex process that began around 4.6 billion years ago with the collapse of a giant molecular cloud. This collapse led to the formation of the Sun at the center, surrounded by a rotating disk of gas and dust. Over time, particles in this disk began to collide and stick together, forming larger bodies known as planetesimals, which eventually coalesced into the planets we know today. As the solar system evolved, processes like accretion and planetary differentiation played crucial roles in shaping the planets. Accretion allowed for the growth of these celestial bodies, while differentiation led to the formation of distinct layers within them. The final stages involved the clearing of debris and the establishment of stable orbits, resulting in the solar system's current structure, which includes the Sun, eight planets, and various other celestial objects.

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Real World Applications