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The protoplanet nebular model is the theory that is most widely accepted to describe the origin of the solar system. The model is made up of 3 stages: A, B, and C. Stage A is the beginning of the creation of the elements that are heavier than hydrogen in previously existing stars. Part 2, stage B, is when the nebula is formed from the raw materials that were created in the first stage, A. With gravitational attraction, the nebula contracts forming the protosun in the center of the nebula. The protosun is then surrounded by a fat, bulging accretion disk around it. The sun forms from the protosun, and the planets form in the accretion disk...
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