Life Cycle of a Star

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  • Created by: H_H
  • Created on: 17-05-17 12:17
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  • Clouds of Dust and Gas
    • Life Cycle of a Star
    • The force of gravity causes the dust and gas to spiral together
      • This forms a protostar
        • Gravitational energy is converted to heat energy
          • When the temperature gets high enough, thermonuclear fusion takes place.
            • The hydrogen nuclei forms helium nuclei
              • This gives out massive amounts of heat and light
                • A main sequence star is formed
                  • This is a long stable period. The heat released by thermonuclear fusion creates outward pressure. This is balanced by the force of gravity, pulling everything in
                    • When the hydrogen runs out, it swells and forms a red giant
                      • A small-to-medium sized star becomes unstable and ejects its outer layer of dust
                        • This creates a planetary nebula
                          • A solid, dense, hot core if left behind. This is a white dwarf. This cools down and eventually fades away
                      • Big stars form a red supergiant
                        • They glow brightly and undergo more nuclear fusion, expanding and contracting several times
                          • Heavier elements are formed in various nuclear reactions
                            • Eventually this will explode to form a supernova
                              • The exploding supernova throws the outer layers of dust and gas into space
                                • This leaves a very dense core called neutron star
                                  • If the star is big enough, it will become a black hole

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