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The formation of a star occurs in three main stages: first, a dense region within a molecular cloud begins to collapse under its own gravity, leading to the creation of a protostar. As the protostar gathers mass and temperature increases, nuclear fusion ignites in its core, marking the transition to the main sequence stage, where the star stabilizes and fuses hydrogen into helium. Finally, once the star exhausts its hydrogen fuel, it will evolve into a red giant or supergiant, eventually culminating in a supernova or the formation of a white dwarf, neutron star, or black hole, depending on its mass.

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4d ago

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