What happens when a red giant star becomes a white dwarf?
A star becomes a white dwarf when fusion reaction stop.
When the fuel runs out and the star's mass falls below approximately eight times that of the sun, carbon fusion cannot be initiated and the star collapses into a white dwarf. At that point, the star is primarily composed of carbon and oxygen and ceases to produce energy through fusion reactions. Initially, the red giant star is fusing hydrogen and helium to produce mostly carbon and oxygen.
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A red giant star that transforms into a white dwarf loses its outer layers, which are ejected into space and form a planetary nebula. The star's remaining core contracts and gets very dense, reaching temperatures of about 100,000 Kelvin. This white dwarf core then cools over billions of years to become a black dwarf because it is no longer undergoing nuclear fusion.
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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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