What is the Color of a Neutron Star?

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SUMMARY

The color of a neutron star is primarily influenced by its temperature and the presence of charged particles. Neutrons themselves are neutral and would be transparent if isolated; however, neutron stars contain a mix of neutrons, protons, and electrons, resulting in a translucent appearance similar to dense fog. The emitted light spectrum varies with temperature, typically appearing blue-white due to extreme heat, which can reach millions of degrees. The discussion highlights the complexity of neutron star composition and the electromagnetic interactions at play.

PREREQUISITES
  • Understanding of neutron star composition and structure
  • Familiarity with Wien's Law and its application to stellar temperatures
  • Knowledge of electromagnetic charge and its relation to transparency
  • Basic principles of quantum mechanics and particle physics
NEXT STEPS
  • Research the effects of temperature on neutron star color using Wien's Law
  • Explore the electromagnetic interactions in neutron stars and their impact on light emission
  • Study the role of electron degeneracy pressure in neutron star stability
  • Investigate the magnetohydrodynamic processes that generate magnetic fields in neutron stars
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Astronomers, astrophysicists, and students interested in stellar evolution, neutron star physics, and the interplay of temperature and electromagnetic properties in dense matter.

  • #31
Jarfi said:
So the ending conclusion is that the neutron "rock" is transparent? that's pretty damn awesome, and than the plasma and maybe hydrogen gas flowing massively hot around the star, blasting white light away... sounds cool to me.

Remember that a neutron star is not composed of ONLY neutrons. The outer layers are mostly protons and electrons. I would bet that a neutron star is not transparent at any wavelength.
 
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  • #32
Are we considering how the star's constituent neutronium would appear close-up or the star as a whole to a faraway observer?

If we talk about the appearance of the star as a whole to an observer in a reference frame further away, then we have to factor in the (significant) gravitational redshift the sheer density of the body creates. One also needs to factor in whether said neutron star has a companion or other source of acreteable material, because acreating material would be accelerated to relativistic speeds, thereby emitting enormous amounts of EM energy. In short, there are more factors beyond simple surface temperature or transparency/lack thereof of the material the star is made of!
 
  • #33
FalseVaccum89 said:
Are we considering how the star's constituent neutronium would appear close-up or the star as a whole to a faraway observer?

If we talk about the appearance of the star as a whole to an observer in a reference frame further away, then we have to factor in the (significant) gravitational redshift the sheer density of the body creates. One also needs to factor in whether said neutron star has a companion or other source of acreteable material, because acreating material would be accelerated to relativistic speeds, thereby emitting enormous amounts of EM energy. In short, there are more factors beyond simple surface temperature or transparency/lack thereof of the material the star is made of!

As I said when I posted this thread, there were two questions involved.

1: the stated question above, the wavelength of light, and combination of different light sources from the neutron star and all factors taken in as a whole for an observer at considerable distance.
2. The interaction of electromagnetic waves with neutrons, picture the neutron star, but no electron clouds.. no plasma and no gas around, just 100% neutrons. The question involved is how will 100% neutrons in 100% density affect light. Will it reflect it all, absorb it all, or not affect it at all due to neutrual charge.

There were multiple factors, including the neutrual charge of a neutron, area charge caused by quarks, the almost nonexistant gaps between the neutrons. and more.
 
  • #34
Jarfi said:
As I said when I posted this thread, there were two questions involved.

1: the stated question above, the wavelength of light, and combination of different light sources from the neutron star and all factors taken in as a whole for an observer at considerable distance.
2. The interaction of electromagnetic waves with neutrons, picture the neutron star, but no electron clouds.. no plasma and no gas around, just 100% neutrons. The question involved is how will 100% neutrons in 100% density affect light. Will it reflect it all, absorb it all, or not affect it at all due to neutrual charge.

There were multiple factors, including the neutrual charge of a neutron, area charge caused by quarks, the almost nonexistant gaps between the neutrons. and more.

I was addressing that to those quibbling over the things I mentioned. Guess I should have specified that! :P

Anyway, the structure of a neutron star isn't going to be 100% neutrons. As far as we know right now, there's going to be an outer 'crust' of regular atomic nuclei in a sea of electrons, an inner 'crust' of the above mixed with superfluid neutrons, and an inner core of superfluid neutrons, superconducting protons, and free electrons. All that's going to make any model of neutron star appearance much more difficult to create. (Reference for specific layer compostion: http://heasarc.gsfc.nasa.gov/docs/objects/binaries/neutron_star_structure.html)
 
  • #35
Chronos said:
Wien's Law is the short answer. Star color is proportional to temperature. Based on this we would expect a neutron star to be in the blue-violet range with some adjustment due to gravitational redshift.

IMHO, all this stuff about black body radiation and surrounding matter is misreading the question. If I asked you "what color is iron" you would not say "Orange" even though orange light does emit from iron at certain high temperatures. "Fresh iron surfaces appear lustrous silvery-gray"- Wikipedia.

The original post asks "What is the colour of pure neutrons confined together?". In other words, Neutronium. As far as I understand it, "Transparent" seems to be the most favored answer here.
 
  • #36
It would not be transparent. The surface is not purely neutron; the pressure is lower at the surface than at the interior. Instead it is made up of nuclei and electrons. In fact throughout the entire neutron star there are still electrons and nuclei, just getting less and less as you get closer to the core. A likely color is gray or black since that's what nuclei + free electrons in an actual material looks like. Most solids are after all just this.
 
  • #37
Algr said:
If I asked you "what color is iron" you would not say "Orange" even though orange light does emit from iron at certain high temperatures.


Well, if you lived somewhere where it was normal for iron to be at that temperature then you would say "orange." The surface of a young neutron star is typically a million degrees, so the natural answer would be bluish white, with lots of X rays, and gamma rays from infalling matter. To me it seems forced to wonder what the surface of the star would look like at "room temperature," but if you want to know...

The astronomers tell us that there is an atmosphere of carbon, probably only a few millimeters thick. There could be an "ocean" of liquid carbon too, though possibly very shallow. So if that was cooled down to ambient Earth temperature it would be ... well, it would depend. If there was the huge pressure of the star you would get diamond. If this were done on Earth you would have black graphite.

So a very old neutron star -- they last forever, as far as anyone knows -- might cool down enough to have a thin surface of diamond. Cool, huh? Or the nuclei might fuse. I dunno.
 
  • #38
If you lived somewhere where it was normal for iron to be at that temperature then you would say "Aaaaa!" and then die.

All materials have the same black body radiation at a given temperature so it makes no sense to describe black body radiation as being a property of the material.
 
  • #39
Lets get rid of the complicated but unrelated stuff like high temperature, iron crust etc.

Assume that strange matter hypotesis is true, so small macroscopic chunk of strange matter is stable. What color reflects that chunk (if it is very cold - 20C)?
 
  • #40
Algr said:
IMHO, all this stuff about black body radiation and surrounding matter is misreading the question. If I asked you "what color is iron" you would not say "Orange" even though orange light does emit from iron at certain high temperatures. "Fresh iron surfaces appear lustrous silvery-gray"- Wikipedia.

The original post asks "What is the colour of pure neutrons confined together?". In other words, Neutronium. As far as I understand it, "Transparent" seems to be the most favored answer here.

Yeah, seems like 70% of the responses here didn't read my question... or they keep saying, durr well yea there are electrons too, yeah I aknowledged that, that was the 1st question, the second was how pure neutronium theoretically behaves alone, in great pressure, and how it interacts with light and such.
 
  • #41
There is no such thing as pure neutronium. If you could somehow get some, it would quickly produce protons and electrons through neutron decay. So this becomes a bit like "what color would gold be if it weren't gold".

Additionally, there seems to be a misconception that light cannot interact with a neutron. That's not true - it can interact magnetically.
 
  • #42
Vanadium 50 said:
There is no such thing as pure neutronium. If you could somehow get some, it would quickly produce protons and electrons through neutron decay. So this becomes a bit like "what color would gold be if it weren't gold".

Additionally, there seems to be a misconception that light cannot interact with a neutron. That's not true - it can interact magnetically.

hmm, there was stated above in this thread, that neutronium exists pressurized in the core of the neutron star, and is mostly neutrons, also if you'd shine a light on it just before it's half life ensue
 
  • #43
Vanadium 50 said:
There is no such thing as pure neutronium. If you could somehow get some, it would quickly produce protons and electrons through neutron decay. So this becomes a bit like "what color would gold be if it weren't gold".

I disagree. For an object to have a definable color, it need only exist long enough to reflect a lone wavelength of red light. (The longest visible to humans, and thus defining "color") Free neutrons have a half life of about 10 minutes. Roentgenium has a similar half life and a predicted color. (Silver)

Edit: Also, is it safe to assume that the half life of neutronium is the same as that of a free neutron?
 
  • #44
Algr said:
I disagree. For an object to have a definable color, it need only exist long enough to reflect a lone wavelength of red light. (The longest visible to humans, and thus defining "color") Free neutrons have a half life of about 10 minutes. Roentgenium has a similar half life and a predicted color. (Silver)

Edit: Also, is it safe to assume that the half life of neutronium is the same as that of a free neutron?

Neutrons in an atomic nucleus have a much longer half life than that. The core of a neutron star is like a huge atomic nucleus, so the half life should be much more than a free neutron.
 

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