How does mass affect star formation?
Available mass determines how fast a proto-star will condense into a star, and what type of star it will be.
This also affects the life-cycle of the star and the final form it will take.
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The gravitational forces inside a molecular cloud are determined by mass, and a higher mass results in stronger gravity, which compresses the material and starts the formation of a protostar.
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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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