Difference between revisions of "Stellar Evolution"

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'''Stellar evolution''' is the theoretical life cycle of a star. It encompasses all aspects of development to the beginnings of a protostar in a [[nebula]] to the emergence of the star on the main sequence to the final stages of its life as a red giant before it degenerates into a [[white dwarf]], [[neutron star]] or [[black hole]].
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'''Stellar evolution''' is the theoretical life cycle of a [[star]]. It encompasses all aspects of development to the beginnings of a protostar in a [[nebula]] to the emergence of the star on the main sequence to the final stages of its life as a red giant before it degenerates into a [[white dwarf]], [[neutron star]] or [[black hole]].
  
 
[[Category:Astronomy]]
 
[[Category:Astronomy]]

Revision as of 14:30, January 30, 2018

Stellar evolution is the theoretical life cycle of a star. It encompasses all aspects of development to the beginnings of a protostar in a nebula to the emergence of the star on the main sequence to the final stages of its life as a red giant before it degenerates into a white dwarf, neutron star or black hole.