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- A review of the beginning & end of stars
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- All stars begin as clouds of dust & gas called NEBULA
- What a star becomes depends on how much mass it has when it starts
- Gravity is the force that begins fusion in stars
- New stars are called protostars
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- An average mass star (like the Sun) has an average life span of 10
billion years
- They convert hydrogen to helium mostly
- They usually can’t fuse any
element larger than carbon
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- When a medium mass star runs out of fuel it increases its size to try to
cool off & prolong its “life” it becomes a RED GIANT
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- Over time a red giant star will be compressed by gravity
- It will try to restart its fusion by heating up
- It will become WHITE DWARF & finally a Black Dwarf (dead star)
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- Stars up to 100 times the mass of the Sun
- Massive stars follow the same life cycle as medium mass stars until
after Red Giant
- Massive stars contain so much energy they create a tremendous explosion
- The explosion is called a SUPERNOVA
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- A massive star core can usually fuse elements up to iron
- After a supernova only the very massive core of the star is left
- This core is called a NEUTRON STAR
- A teaspoon of neutron star material is so dense it would have a mass of
100 million tons
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- A Supermassive star (over 100 times the sun’s mass) has the same “life
cycle” as a massive star
- The difference is that a Supermassive star becomes a BLACK HOLE
- Scientists believe that there is a black hole at the center of every
spiral & elliptical galaxy
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- A black hole is where the core is so massive after the supernova that it
collapses in upon itself
- It becomes a “cosmic vacuum cleaner” sucking even light into it
- The only way we detect black holes is by x-rays or light given off by
something being sucked into it.
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