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Published byCharlene Boyd Modified over 6 years ago
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The lifecycle of a star This Photo by Unknown Author is licensed under CC BY
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Interstellar Medium The total mass of gas and dust between stars
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Stellar Nebulae A cloud of gas and dust where new stars are born
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Protostar The birth of a star caused by the collapse of dense regions in a nebula due to gravity.
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Main sequence star The longest, most stable period of a star’s life where it converts hydrogen to helium in its core, generating heat and light.
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Red Giant As the core runs out of hydrogen and helium, the outer layers of the star expand, cool, and become a dimmer red colour.
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Planetary Nebula Occurs at the end of a red giant’s life when the outer layers of the star start to drift off into space.
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When a red giant collapses, its outer layers shed off and what remains is a very hot, dense star.
White Dwarf
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Giant star 100 times larger and 1000 times brighter than a normal main-sequence star of the same surface temperature
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Red supergiant After the hydrogen in a giant star's core has been used up, they become the largest stars in the universe.
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After the hydrogen in a giant star's core has been used up, they become the largest stars in the universe. Supernova
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Black hole Click image for Brian Cox’s explanation of a Black Hole Created when a giant star undergoes a supernova, its an object so dense that not even light can escape its gravity.
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If the mass of a supernova core is not large enough, it forms a star made entirely of neutrons instead of a black hole. Neutron star
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