How to Calculate Average Atom Separation in the Sun's Core?

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SUMMARY

The discussion focuses on calculating the average separation of atoms in the Sun's core using the Saha equation and the radius of the first Bohr orbital. Participants clarify that for fully ionized hydrogen, the number density of hydrogen atoms equals the electron density. The conversation emphasizes that if the average separation calculated from electron density equals twice the Bohr radius, it indicates a predominance of non-ionized hydrogen. However, the consensus acknowledges the complexity of the solar core's composition, which consists of charged particles and free electrons.

PREREQUISITES
  • Saha equation for ionization equilibrium
  • Understanding of Bohr model and Bohr radius
  • Concept of electron density versus atom density
  • Basic principles of nuclear fusion in stellar cores
NEXT STEPS
  • Research the implications of the Saha equation in stellar astrophysics
  • Study the relationship between electron density and atomic density in plasmas
  • Learn about the conditions in the solar core and nuclear fusion processes
  • Explore advanced topics in quantum mechanics related to atomic separation
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Astronomy students, astrophysicists, and researchers interested in stellar physics and the dynamics of the solar core.

lycraa
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Homework Statement


in part 1 i used the Saha equation to calculate that the hydrogen in the center of the sun was fully ionized (given temperature and central electron density). part 2 says:

Re-examine the result by computing the average separation of atoms at the center of the sun knowing the radius of the first Bohr orbital.




I'm a little lost here. this would be no problem if i was given the atom density, but I'm not sure how to deal with the electron density
 
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lycraa said:

Homework Statement


in part 1 i used the Saha equation to calculate that the hydrogen in the center of the sun was fully ionized (given temperature and central electron density). part 2 says:

Re-examine the result by computing the average separation of atoms at the center of the sun knowing the radius of the first Bohr orbital.




I'm a little lost here. this would be no problem if i was given the atom density, but I'm not sure how to deal with the electron density

How many electrons are there per atom, for hydrogen? What does that tell you about the number density of hydrogen atoms, given the number density of electrons?
 
well, for NON ionized hydrogen, you would have only one electron. meaning that the number density would be the same as the electron density. So would i be right in saying then, that if the average separation i found using the electron density equals 2* bohr radius, i would have mostly non ionized hydrogen?
 
lycraa said:
well, for NON ionized hydrogen, you would have only one electron. meaning that the number density would be the same as the electron density.

I'm not sure why you have "NON" in all caps. I mean, if you take hydrogen and ionize it, you're still going have equal numbers of protons and electrons. Extra electrons don't just appear out of nowhere.

lycraa said:
So would i be right in saying then, that if the average separation i found using the electron density equals 2* bohr radius, i would have mostly non ionized hydrogen?

I'm sorry, but I don't know the answer to that. On the one hand, this does seem to be the tree up which this problem is barking, by having you reconsider your previous result, and showing that these supposedly "free" electrons don't have much room to move around. On the other hand, I had always thought that the solar core consisted of charged particles, especially since people always talk of the fusion reaction consisting of free protons combining together to form helium nuclei. Besides, although those electrons may, on average, have a mean free path that is not much larger than the orbital of a bound electron, they are still too energetic to remain bound, which would have me lean more towards the ionized picture. EDIT: Remember that I said that I just don't know for sure.
 

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