Dark Matter Stars: Burning Hot and Invisible

Click For Summary
SUMMARY

The discussion centers on the concept of dark matter stars and their relationship to stellar temperatures and emissions. Participants clarify that while hotter stars emit more radiation, they cannot become invisible through heating; instead, they would appear brighter. Dark matter, which does not clump and cannot form stars, is fundamentally different from stellar objects. The conversation also references the detection of distant astronomical objects in the X-ray and gamma-ray spectrum, emphasizing that dark stars, speculated to exist in the early Universe, would be cold and undetectable due to low-frequency emissions.

PREREQUISITES
  • Understanding of stellar temperatures and radiation emissions
  • Familiarity with dark matter concepts and properties
  • Knowledge of electromagnetic spectrum and detection methods
  • Basic principles of Wien's displacement law
NEXT STEPS
  • Research the properties of dark matter and its implications in astrophysics
  • Learn about stellar evolution and the life cycle of stars
  • Explore detection methods for X-ray and gamma-ray astronomical objects
  • Investigate the theories surrounding supermassive black holes and dark stars
USEFUL FOR

Astronomy enthusiasts, astrophysicists, and students interested in the nature of dark matter and stellar physics will benefit from this discussion.

presto129
Messages
2
Reaction score
3
ok so this has been on my mind for a while. If the hotter a stars burn or flame the further it goes on the spectrum correct so what if it burned so hot it is literally invisible wouldent that be considered a dark matter then it's a dark matter sun
 
  • Like
Likes   Reactions: hsdrop
Astronomy news on Phys.org
presto129 said:
ok so this has been on my mind for a while. If the hotter a stars burn or flame the further it goes on the spectrum correct so what if it burned so hot it is literally invisible wouldent that be considered a dark matter then it's a dark matter sun
If it emits electromagnetic waves, then we would see it. And a star always does. Even the cold ones, the hottest the more. It doesn't matter whether the emissions are in the visible spectrum or not. This is not what is meant by dark matter. Dark matter is something completely different, and we don't know much about it. To the few we do know belongs the fact, that dark matter doesn't clump and therefore cannot build stars.
 
  • Like
Likes   Reactions: presto129
fresh_42 said:
If it emits electromagnetic waves, then we would see it. And a star always does. Even the cold ones, the hottest the more. It doesn't matter whether the emissions are in the visible spectrum or not. This is not what is meant by dark matter. Dark matter is something completely different, and we don't know much about it. To the few we do know belongs the fact, that dark matter doesn't clump and therefore cannot build stars.
I'm in 8th grade thanks still learning love physics and astronomy
 
  • Like
Likes   Reactions: stoomart and hsdrop
presto129 said:
I'm in 8th grade thanks still learning love physics and astronomy
You're welcome, and by the way

:welcome:

Have fun!
 
  • Like
Likes   Reactions: presto129
fresh_42 said:
the hottest the more

Some very hot very distant astronomical objects are only detectable in the X-ray and gamma-ray spectrum. The visible light they emit is just too feeble to detect from Earth while the higher wavelengths are much stronger.

Here is one of the beasties we use to see these:

http://chandra.harvard.edu/

BoB
 
It has been speculated that dark stars with a high amount of dark matter inside existed in the early Universe (https://arxiv.org/abs/0705.0521). However, these objects would be very cold and therefore not be detectable as the emitted radiation would be very low frequency. They would be kept from collapsing by dark matter annihilations.

Note that you cannot make something invisible by heating it. Although the peak of the emission spectrum would shift to unobservably high frequencies, the total emission would increase in such a way that the emission in the visible sector would increase rather than decrease, ie, it would become even brighter. The way of obtaining an object whose EM radiation cannot be seen is to make it cold so that the intensity decreases. Dark matter is a different issue, it does not emitt EM radiation at all (or very very very weakly).
 
  • Like
Likes   Reactions: stoomart and mfb
presto129 said:
ok so this has been on my mind for a while. If the hotter a stars burn or flame the further it goes on the spectrum correct so what if it burned so hot it is literally invisible wouldent that be considered a dark matter then it's a dark matter sun
Hotter objects emit more radiation than colder objects - for every wavelength range.

We can detect gamma rays without an upper energy limit - at high energies they just get too rare to measure their rate reliably, but if there would be something emitting them often we would easily see it.

Stars cannot get too hot - otherwise the intense radiation pressure would quickly remove their outer shells, cooling the star.

We know that dark matter has a different distribution than visible matter. It does not clump together like visible matter does - it cannot be in star-like objects (at least not most of it).
 
presto129 said:
ok so this has been on my mind for a while. If the hotter a stars burn or flame the further it goes on the spectrum correct so what if it burned so hot it is literally invisible wouldent that be considered a dark matter then it's a dark matter sun
The hotter the star, the further on the spectrum is the peak radiation intensity. For any wavelength, intensity increases with temperature. It's just that as stars get hotter, larger proportion of light is in the shorter wavelengths, making the star look bluer.
Below is the black body spectrum, which closely approximates stellar output:
720px-Wiens_law.svg.png

As you can see, it 'leans' to the left with increasing temperature (as described by Wien's displacement law). You can imagine a body so hot, that its peak wavelength is way in the gamma range. It would still look blue, since that's where the most intensity in the visible range (~400-800 nm) would be radiated.

(edit: so many ninjas! ;) )
 
rbelli1 said:
Some very hot very distant astronomical objects are only detectable in the X-ray and gamma-ray spectrum. The visible light they emit is just too feeble to detect from Earth while the higher wavelengths are much stronger.
Or hot and small. Such as neutron stars.
 
  • Like
Likes   Reactions: rbelli1
  • #10
presto129 said:
I'm in 8th grade thanks still learning love physics and astronomy
I'm 34 and just starting learning this stuff, learned a lot from these guys and learn a ton more everytime I visit these forums. Good luck in your learning and don't ever stop asking questions or looking for answers, hope you stick around.
 
  • #11
Orodruin said:
It has been speculated that dark stars with a high amount of dark matter inside existed in the early Universe (https://arxiv.org/abs/0705.0521). However, these objects would be very cold and therefore not be detectable as the emitted radiation would be very low frequency. They would be kept from collapsing by dark matter annihilations.
They were talking about these giant dark matter stars on How The Universe Works as a candidate for the source of supermassive black holes, any credibility to this?
 

Similar threads

  • · Replies 42 ·
2
Replies
42
Views
4K
  • · Replies 49 ·
2
Replies
49
Views
5K
  • · Replies 7 ·
Replies
7
Views
2K
  • · Replies 21 ·
Replies
21
Views
3K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 0 ·
Replies
0
Views
3K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 10 ·
Replies
10
Views
5K
  • · Replies 13 ·
Replies
13
Views
4K
  • · Replies 9 ·
Replies
9
Views
1K