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Evolution of Stars
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Main Factor of Life Cycle
Beginning mass
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Nebulae Huge clouds of dust and gas
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M16 – Eagle Nebula
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M16 – Eagle Nebula
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Stars forming in Trifid Nebula M20
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½ light year long twisters in Lagoon Nebula M8 in Sagittarius
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Protostar Hot, contracting cloud of dust and gases
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When the temp. reaches 10,000,000 °C, a star is born
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Star forming region in NCG 2366
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Star forming region of NCG604
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Medium-sized Stars Most common star type Our sun
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Red Giant Most of the hydrogen is used up Outer shell begins to expand
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As it expands, it cools and becomes red
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Core gets hotter – up to 200,000,000 °C – where helium is fused into carbon
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Gas drifts off forming a planetary nebula
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Eskimo Nebula – NCG2392
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MyCn18 – young planetary nebula 8000 light years away
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Stingray Nebula – youngest nebula known
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Ring Nebula – planetary nebula around a white dwarf
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White Dwarf Extremely dense White hot
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M4 – comparison of ground based observation to HST
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Massive Stars Start like medium-sized stars
Become supergiants after red giant stage
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Temp can reach 600,000,000 °C Carbon atoms fuse and eventually form iron
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Betelgeuse – red supergiant
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Supernova Tremendous explosion Heat can reach 1,000,000,000 °C
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Iron atoms fuse to form heavier elements
Can light up our sky
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Southern Crab Nebula
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Supernova remnant – Veil Nebula – NGC6992
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Neutron Stars Often less than 16 km in diameter Spin very rapidly
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Energy is given off in narrow beams
Pulsars – appear to give off pulses of energy
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2 X-ray pulsars, Geminga and Crab Pulsar
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Neutron star
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Black Holes Incredibly massive stars
Gravity becomes so strong that even light cannot escape
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Artist concept of a black hole
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Black hole candidate in M87
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Black hole in NGC4261
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