How does the Sun's mass affect its evolution?
It determines its life span and the stages therin.
The opposite is true for smaller stars, which have longer lifespans due to their greater instability; our sun is an example of an average star with an average lifespan.
Lighter stars may simply explode, fizzle out, or lose their outer shell or atmosphere. Heavier stars will explode or collapse on themselves in a way that results in a supernova, black hole, or planetary nebula. A star's mass also plays a role in the outcomes of the star "dying."
By signing up, you agree to our Terms of Service and Privacy Policy
Elevated mass leads to a shorter and more intense lifecycle, with a faster main-sequence phase and eventual transition to a red giant and supernova. The Sun's gravitational forces, internal temperature, and nuclear fusion rate are all influenced by mass.
By signing up, you agree to our Terms of Service and Privacy Policy
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.
- 98% accuracy study help
- Covers math, physics, chemistry, biology, and more
- Step-by-step, in-depth guides
- Readily available 24/7