What is the next stage of the sun's evolution?
Sun is a main sequence star now. It will become red giant and then white dwarf after 5 billion years.
Sun is a main sequence star now. After about 5 billion years it will become red giant and finally a white dwarf.
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The red giant phase is the next stage of the Sun's evolution.
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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.
- What physical process generates a force inside a pre-main-sequence star to offset the force of gravity and stop the star from slowly condensing and shrinking, thus producing a stable, non shrinking main-sequence star?
- What are protoplanetary objects?
- What is the revolution period of the sun in years?
- What is a structure of the star?
- What is a stars rotational symmetry?
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