Summary
Stars are born from massive clouds of dust and gas collapsing under their own gravity and fuse hydrogen atoms to form helium. The destiny of a star is determined by its initial mass. As stars deplete their hydrogen fuel, they progress to fusing heavier elements like carbon and oxygen. Eventually, stars can expand and shed outer layers, leaving behind dense cores. Massive stars end their life in supernova explosions, giving rise to neutron stars.
Formation of Stars
Stars are formed from huge clouds of dust and gas collapsing under their own gravity, fusing hydrogen atoms to create helium.
Life Cycle of Stars
The future of a star depends on its mass at birth. After fusing hydrogen into helium, stars like the sun start fusing heavier elements like carbon and oxygen.
End of a Star's Life
As stars run out of hydrogen, they start fusing helium, growing larger and eventually shedding their outer layers to become dense cores. Massive stars end in supernova explosions, forming neutron stars.
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