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Star Formation Stars form by a collection of dust and debris - that end up becoming a dense collections of gas that is known as molecular clouds. These regions are extremely cold ( usually about 10 to 20K, above absolute zero.) The most common atoms that form stars is CO and H2. The denseness of the clouds can also cause gas to clump together into high densities and when these densities become high enough a star is born.
Created and Edited by Ariel |
HR ChartMore information on the HR diagrams and their role in star formation.
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Types of StarsMore information on the types stars that are a possible result of star formation.
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Spectral ClassFind out what spectral class the stars fall under.
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