It's All About Mass
All stars are born, mature, and eventually die. A star's mass determines how it will live and die (mass is the amount of matter contained in something).
Throughout the universe, stars are born in dense clouds of gas and dust. Gravity pulls the gas and dust into clumps. If the clump is massive enough, a star can form! The growing temperature and pressure causes its core to ignite and nuclear fusion begins.
After millions to trillions of years, a star will begin to run out of fuel. What happens next depends on its mass. The least massive stars will swell into red giants. They will eject their outer layers and their cores will shrink into small white dwarfs. Massive stars will swell into red or yellow supergiants before ejecting their outer layers. Then they will collapse in on themselves and explode as supernovas. The remaining cores shrink into small neutron stars. The most massive stars form black holes after they explode in super-novas. Black holes are so dense that not even light can escape their gravity!