Difference between revisions of "Nebula hypothesis"
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| − | The '''nebula hypothesis''' is a model of the formation of a solar system. It theorizes that a solar system begins as a rotating cloud of gas and dust that contracts to create a flat disk with a star at its center. | + | The '''nebula hypothesis''' (alternately, '''nebular hypothesis''') is a [[Big Bang]] theory model of the formation of a [[solar system]]. It theorizes that a solar system begins as a rotating cloud of [[gas]] and [[dust]] that contracts to create a flat disk with a [[star]] at its center. [[Planet]]s grow from the [[particle]]s surrounding the star, creating a solar system. |
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| + | [[Category:Astronomy]][[Category:Physics]] | ||
Revision as of 21:01, June 24, 2008
The nebula hypothesis (alternately, nebular hypothesis) is a Big Bang theory model of the formation of a solar system. It theorizes that a solar system begins as a rotating cloud of gas and dust that contracts to create a flat disk with a star at its center. Planets grow from the particles surrounding the star, creating a solar system.