
The Life Cycle of a Star: From Nebula to Supernova
A star is a self-gravitating ball of hot gas (plasma) that shines because its core releases energy through nuclear fusion. The “life cycle of a star” is the story of how that balance begins inside a cold nebula, settles into a long stable phase, and—if the star is massive enough—ends with a supernova that reshapes its neighborhood.[a]↗ A Simple Way to Hold the Whole Story… The Life Cycle of a Star: From Nebula to Supernova








