Is it true that stars the size of the sun will never have a core hot enough to fuse carbon?
Yes, stars the size of the Sun aren't hot enough for carbon fusion.
The star expands into a red giant at this point, collapsing until hydrogen fusion can begin in the region outside the core when the hydrogen in the core runs out.
When a star has less mass than eight times that of the Sun, its helium supply runs out and it becomes a white dwarf star with an oxygen-carbon core that is incapable of undergoing further fusion reactions.
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It is true that a star's core will never get hot enough to fuse carbon, even for stars the size of the sun.
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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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