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III. Stellar Evolution You’re a Superstar! 1. 1st Step: a. Stars form from nebulas (cloud of dust & gas) 2. 2nd Step: a. As nebula contracts, a small star is formed called a protostar b. Eventually, the protostar will begin nuclear fusion (elements coming together) 3. 3rd Step: a. Star joins the main sequence 1.) 90% of stars spend life here Life Cycle of Stars 4. 4th Step: a. What stars end up as depend on mass b. Low mass = red giant (massive star, a lot of fusion) c. High mass = supergiant (largest known star, burn out fast) 5. Death of Stars: a. Low and Medium mass stars • Planetary nebula --------- white dwarf (dense, faint star)------ black dwarf (dead star) b. High mass stars • Supernova (exploding star) --------- neutron star(remains of star) or black hole (massive gravity absorbs everything near it) Relative Size of Stars to Planets Earth Science Bellringer • Get out your comp. books! Star Life Cycle Diagram Using pg. 764-765 draw a DETAILED & LABELED diagram of the star life cycle in your composition notebook. Red textbook Star Life Cycle Questions: 1. 2. 3. 4. 5. 6. 7. What is a nebula? How does a star form from a nebula? How is a protostar different from a star? What factors determine how long a star lives? What is the ultimate fate of our sun? What type of stars may become black holes? Describe the difference between a white dwarf and a black dwarf. 8. Describe the two alternatives for a supernova.