1. THE LIFE OF A STAR http://hubblesite.org/newscenter/archive/releases/nebula/2004/26/

2. What will determine how a star lives out its life? ( Examine the diagram.) How much mass a star has. What is mass? How much matter is present in a given object.

3. (1) Nebula (http://www.meade.com/gallery/images/orion_nebula.jpg)

4. Nebula: A cloud of gas and dust where stars are born!

5. (A) First Contraction: Gravity pulls together gas and dust which causes the particles to condense an heat up.

6. (2) Protostar http://physics.ship.edu/~mrc/pfs/108/node3.htm

7. Protostar: The first star formed where fusion occurs due to the condensing of the particles and energy is radiated outward.

8. Fusion: The combining of two atomic nuclei which produces large amounts of heat. Example: hydrogen + hydrogen = helium + heat

9. (3) Main Sequence http://physics.ship.edu/~mrc/pfs/108/node3.htm

10. Main Sequence Star: A middle-aged stable star which uses hydrogen as a fuel source. The inward force of gravity equals the outward force of fusion and the star remains stable. Example: The Sun

11. http://physics.ship.edu/~mrc/pfs/108/node3.htm

12. (B) Second Contraction: The outflow of energy from the fusion of hydrogen is less than the gravity keeping the star together.

13. (C) Expansion: The star starts to fuse helium and this creates the release of energy which is greater than the force of gravity.

14. (4) Red Giant

15. Red Giant http://wonderquest.com/images/2005-03-10-red-giant-star.jpg

16. Red Giant: A large, bright, cool star which uses helium as a fuel source.

17. (D,E,G) Third Contraction The supply of helium is depleted which causes the force of gravity to be greater than the energy released from the star due to fusion.

18. If the amount of matter in the star is average (up to 8 times the Sun’s mass),it will follow Path #1 to form a White Dwarf (5). A White Dwarf: a small,dim,hot star. A White Dwarf will eventually burn out and form a Black Dwarf (6).

19. White Dwarf http://www.astronomy.mps.ohio-state.edu/npogge/Ast162/unit3/extreme.html

20. http://leonatopo.splinder.com/archive/2005-12

21. Nova: A star that changes in brightness and has an explosion which removes some of its outer layers.

22. If a star is more massive than the sun ( 8 to 20 times greater ),during the 3 rd Contraction, the outer layers will violently explode and implode, throwing matter into space as well as creating a dense core. This phenomenon is called a: Supernova (F,H).

23. Supernova http://historyoftheuniverse.com/hotuwiki/index.php/Supernovahttp://historyof

24. Supernova: A violent explosion which occurs within the outer layers of a massive collapsing star which throws matter into space as well as implodes matter into the middle forming a dense core.

25. The end result: A Neutron Star (7)

26. Neutron Star http://solarsystem.nasa.gov/multimedia/gallery/neutron.jpg

27. Neutron Star: A star that forms from a collapsed star which had 8 to 20 times the mass of our Sun. Smaller and denser than a White Dwarf.

28. Neutron Star – Pulsar http://stardate.org/images/gallery/neutron_star.jpg

29. If the star is an extremely massive star (greater than 20 Sun masses), during the 3 rd Contraction, a supernova will occur which will create a collapsed star so dense, visible light will not be able to leave its gravitational pull. This is called a --?

30. Black Hole (8) http://brokekid.net/img/blackhole.jpg

31. Black Hole: A collapsed star so dense that visible light cannot escape its gravitational pull.