Imagine you could watch a star cluster from the time of its birth to an age of 13 billion years. What you would see happening during that time?
A star's life span is much more than 10 billion years. It would pass through various stages, from nebula to ( ,perhaps, the current stage) supernova or neutron star or Black Hole.
There seems to be a brief window of grace between B instant and
star formation.
But the phases of transition are
Blue star to nebula to blue-white supergiant
star to neutron star to supernova to black hole.
The Sun, our star, is only 4.6 billion years old (by). It could eventually turn red.
giant by roughly the tenth and turn into a black dwarf later.
The Sun is not in the middle ages; rather, it is currently in a high-
lively forties in people.
By signing up, you agree to our Terms of Service and Privacy Policy
In the 13 billion years that you would observe a star cluster, you would see different stages of stellar evolution: the cluster would form from a cloud of gas and dust; stars would be born within the cluster, go through their main sequence phase where they burn hydrogen; eventually, some stars would explode as supernovae, enriching the interstellar medium with heavy elements; the cluster would gradually lose its brightest and most massive stars through stellar winds or supernova explosions; and finally, after billions of years, the cluster would contain mostly low-mass stars, and it might disperse
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.
- How does the pulsation of cepheid variables allow astronomers to estimate age?
- How would you use the parallax formula to determine the distances to a star (in parsecs)? The parallax angle is 0.001293.
- What does a super massive stars end up as?
- What is the life cycle of a star?
- How does gravity affect our galaxy?

- 98% accuracy study help
- Covers math, physics, chemistry, biology, and more
- Step-by-step, in-depth guides
- Readily available 24/7