How does a star change over its life cycle?
To quote Hemingway on 'How did you go bankrupt?':
'Two ways. Gradually, then suddenly.'
First we need to define the 'birth' of a star. Stars are created when giant molecular clouds starts collapsing into a small core (think a few thousand times the Solar System) .
NOT TO SCALE) with heavier elements closer to the center (they're heavier so they sink). This is a star that only has a few days to live as it's already accumulated inert iron in its centre.
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Before a star can become a main sequence star, it must first collapse into a cloud of gas and dust, ignite nuclear fusion, and become a protostar. Depending on how massive the star is, it can then become a red giant, shed its outer layers as a planetary nebula, and leave behind a white dwarf. Stars that are more massive can explode into supernovae, which can result in neutron stars or black holes.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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