Limitation to mass of currently forming stars?

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In summary, the state of our universe contains enough matter to prevent radiation from young stars from interacting with it, leading to the exclusion of stars more massive than the Sun from forming. However, this limit is much higher than a solar mass and may only apply in certain environments.
  • #1
Holocene
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Is this true or false?

The state of our universe, as it is today, contains enough matter comprised of heavy elements, that the radiation from young stars will interact with this matter in such a way that it will be prevented from nearing the star, and thus the mass of the star, and all currently forming stars, will never be able to attain a mass as great as even our own sun.
 
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  • #2
Holocene said:
Is this true or false?

The state of our universe, as it is today, contains enough matter comprised of heavy elements, that the radiation from young stars will interact with this matter in such a way that it will be prevented from nearing the star, and thus the mass of the star, and all currently forming stars, will never be able to attain a mass as great as even our own sun.

False. Photons interacting with atoms may ionize the atoms, but have essentially no effect on the nuclei, which would fall in due to gravity.
 
  • #3
Holocene said:
The state of our universe, as it is today, contains enough matter comprised of heavy elements, that the radiation from young stars will interact with this matter in such a way that it will be prevented from nearing the star, and thus the mass of the star, and all currently forming stars, will never be able to attain a mass as great as even our own sun.

It is false, but only because of the last bit, "will never be able to attain a mass as great as even our own sun". The presence of heavy metals is thought to impose an upper limit on the mass of newly-formed stars, but the limit is much higher than a solar mass and depends on upon the environment in which the star formed.


mathman said:
False. Photons interacting with atoms may ionize the atoms, but have essentially no effect on the nuclei, which would fall in due to gravity.

The photons have momentum, so there will be radiation pressure. Regardless of whether this pressure is imparted to the electrons, atoms, or ions, it can still act to prevent infall or blow material outwards because electromagnetic forces are constantly acting to keep the plasma neutral.
 
  • #4
Stars more massive than the Sun tend to burn out in a few million years. Yet we observe pleantly of stars more massive than the Sun. This implies they were formed recently. So you can think of your question in a statistical sense. If this cut-off were real, what are the odds in this 15-billion-year-old universe that the cut-off was reached in the last few million years?
 
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1. What is the maximum mass that a star can attain?

The maximum mass that a star can attain is around 150 times the mass of the Sun. This is known as the Eddington limit, which is the point at which the outward radiation pressure from the star's energy production is balanced by the inward force of gravity.

2. Why do stars have a limit to their mass?

Stars have a limit to their mass because once a certain amount of matter is accumulated, the inward force of gravity becomes so strong that it overcomes the outward pressure from the star's energy production. This creates a balance and prevents the star from becoming any larger.

3. Can stars with more mass form?

No, stars with more mass cannot form. As mentioned before, the Eddington limit prevents stars from growing any larger. Additionally, the intense radiation and strong stellar winds from high-mass stars can disrupt the formation of other stars in their vicinity.

4. How do scientists determine the mass of forming stars?

Scientists determine the mass of forming stars by studying their spectral signatures. The amount of light emitted by a star at different wavelengths can reveal its temperature, luminosity, and mass. They also use mathematical models and simulations to estimate the mass of forming stars.

5. Can the mass limitation of stars change over time?

Yes, the mass limitation of stars can change over time. As stars evolve and go through different stages of their life cycle, their mass can change. For example, a star may lose mass through strong stellar winds or gain mass through accretion of matter from a companion star.

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