How massive/hot does a star have to be for fusion to occur

In summary, the process of star formation involves the accretion of matter until a critical mass of approximately 80 times Jupiter's mass is reached, at which point nuclear fusion is ignited due to the high temperatures in the core. The minimum mass of hydrogen needed for fusion to occur is about 0.13 solar mass and quantum tunneling is responsible for allowing fusion to occur at this mass. While nuclear reactions can occur without tunneling, it greatly increases the reaction rate by allowing particles with lower energies to fuse.
  • #1
ugalpha
22
0
without having to rely on quantum channeling
 
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  • #2
The basic process of star formation is that they emerge due to accretion of enough matter to reach a critical mass* of approximately 80 times Jupiter's, at which point internal pressures raise the core temperatures high enough to ignite nuclear fusion.
The core has to get to about 15 million K, although some say about 10 million K.
http://burro.cwru.edu/stu/advanced/stars_birth.html

The sun's mass is about 1048 times the mass of Jupiter, so a mass of hydrogen must have about 0.13 solar mass to start fusion with the pp-chain. This assumes that the cloud from which the star forms is mostly hydrogen.

http://www.duke.edu/~teb/stars/nebula.html

http://abyss.uoregon.edu/~js/ast222/lectures/lec11.html

On the distribution of protostar masses by Philip C. Myers - http://arxiv.org/abs/0910.3120 - or -
http://arxiv.org/ftp/arxiv/papers/0910/0910.3120.pdf

See also - http://iopscience.iop.org/0004-637X/687/1/340/fulltext/75147.text.html
 
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  • #3
ugalpha said:
without having to rely on quantum channeling

Are you referring to Quantum Tunneling? I've never heard of Quantum Channeling.
 
  • #4
can fusion at 0.13 solar masses occur without quantum tunneling?

infact can nuclear reactions occur without tunneling or can sufficent kinetic energy convey enough energy to get nuclei into actual contact?
 
  • #5
goldsax said:
can fusion at 0.13 solar masses occur without quantum tunneling?

I don't believe so. Even at 1 solar mass quantum tunneling is responsible for allowing the proton-proton chain to start by allowing two protons to tunnel close enough to each other for fusion to occur.

infact can nuclear reactions occur without tunneling or can sufficent kinetic energy convey enough energy to get nuclei into actual contact?

Yes, however tunneling will always increase the reaction rate by allowing nuclei that wouldn't normally have enough energy to overcome the columb barrier tunnel through. Even at temperatures high enough for fusion to occur without tunneling, the temperature is only an average. Some particles will be higher and some will be lower. Tunneling allows some of those that are lower to fuse.
 
  • #6
ugalpha said:
without having to rely on quantum channeling

Why even ask? Seems like a pointless question.
 
  • #7
qraal said:
Why even ask? Seems like a pointless question.

I forgot to add that the potential barrier in p-p fusion is the equivalent of ~10 billion K. That's far too high to occur in any star without tunnelling. And is also why p-p fusion is so very, very slow. Fortunately for all life on Earth.
 

What is nuclear fusion?

Nuclear fusion is a process in which two or more atomic nuclei combine to form a heavier nucleus, releasing energy in the process.

What is the temperature required for fusion to occur?

The temperature required for fusion to occur is extremely high, typically around 10 million Kelvin (K) or higher. This is because the high temperature is needed to overcome the repulsive force between positively charged nuclei and allow them to fuse together.

What is the mass required for fusion to occur?

The mass required for fusion to occur varies depending on the type of nuclei involved. Generally, larger nuclei require higher temperatures to fuse, but the exact mass required also depends on the pressure and density of the material.

Can any star undergo fusion?

No, only stars with a certain mass and composition are able to undergo fusion. Generally, stars need to have a mass of at least 0.08 times that of our Sun in order to sustain fusion reactions in their cores.

What happens if a star is not massive enough for fusion to occur?

If a star is not massive enough for fusion to occur, it will not be able to sustain itself and will eventually cool and shrink, becoming a brown dwarf or a white dwarf depending on its initial mass and composition.

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