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Life Cycle of a Star
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Nebula Baby star Composed of gas and dust
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Protostar Center of nebula begins to shrink as it gets hotter
Nuclear fusion begins
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Main Sequence “Middle Age”
Star will spend most of its life in this stage
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Red Giant Star starts to die It expands 1,000 times its original size
No more nuclear fusion (no more hydrogen) Fun Fact: Our Sun will expand 400x its current size
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Planetary Nebula Star blows off its outer layer of ionized gases off into space
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White Dwarf Gravity crushes the matter into small planet-sized body of immense density VERY BRIGHT
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Black Dwarf Dead Star Ball of gas not capable of nuclear fusion within its core **Theoretical: The universe is not old enough for the first white dwarf to have burned out **
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Draw the Bohr models for:
Helium Carbon Sulfur
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Nebula Baby star Composed of gas and dust
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Protostar Center of nebula begins to shrink as it gets hotter
Nuclear fusion begins
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Main Sequence “Middle Age”
Star will spend most of its life in this stage
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Red Supergiant MORE mass = MORE hydrogen = MORE energy
Run out of Hydrogen faster (larger)
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Supernova Violent death of high mass star
Occur when nuclear fusion can no longer produce heat required for equilibrium Star collapses and then EXPLODES
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Neutron Star Very dense
Collapsed core of supernova is 2x the size of the sun Shrinks to 20 km in size with the density of 1 tsp weighing 100 million metric tons
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Black Hole Collapsed supernova core is 3x more massive than the sun
Incredibly dense object Gravity is so strong that not even visible light can escape from it
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Our sun will not explode! It is not a massive star
Remember…. Our sun will not explode! It is not a massive star
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Draw and Copy
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