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Describe the life cycle of a small mass star.
All stars are born from nebulae, and small mass stars are no different. Once the star has formed, it is called a Main Sequence star. After a certain period of time, it will burn through all of its Hydrogen, and expand to form a Giant star. Once it burns through all heavier elements (Helium, etc.) all nuclear fusion will cease. At this point, the gravity of the star will cause the core to collapse, while the star's atmosphere drifts away, forming a planetary nebula. Once the star's atmosphere has drifted away, all that is left is the white hot core, called a white dwarf. Finally, once the white dwarf has cooled completely, it is a cold, dark black dwarf star.