Why not fewer visible stars in far away galaxies?

In summary, the person dropping the object would measure that it took half a second for the object to fall from a height of 10 meters, even though according to his clock it only took one second for the object to fall from the same height on Earth.
  • #1
helix_angle
4
0
Hello,
I have a question concerning general relativity. (go easy - I have only knowledge from general consumption physics books). Something curious I have been thinking about requires an explanation as to where I am incorrect in my thinking:

My understanding is that, as something moves relative to an observer, the speed at which it moves constitutes its energy, and therefore its mass. Since mass curves space-time, the amount of curvature an object causes (i.e. the gravitation pull caused by its mass) must be also be relative to the observer. This seems to me absolutely bizarre - but pressing on:

Assuming the above is correct then: At some point approaching the speed of light the mass an object relative to an observer must reach the point where photons reflected from its surface can no longer escape its mass, causing it to appear to the observer to be a black hole (invisible), where for another observer moving with the object it would appear perfectly normal.

Then would it also not be true that what we indirectly detect to be black holes in galaxies far away that are rushing away from us (the further the faster with accelerating space-time expansion) may actually not be black holes but normal (if large) stars relative to an observer in the same galaxy? Therefore the number of "visible" stars in galaxies far enough away should appear to be less and less, but I haven't read anywhere that this is the case. Why?


Thanks,
Helix_Angle
 
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  • #2
No, when objects recede from us, they emit the same number of photons - the only change is in the frequency (they are red-shifted). Now due to the inverse square law, we see more distant objects as dimmer, but only as a function of distance, not as a function of recession speed.
 
  • #3
you didn't read my question properly. I was asking whether general relativity provides that at some point approaching the speed of light the mass an object relative to an observer must reach the point where photons reflected from its surface can no longer escape its mass, causing it to appear to the observer to be a black hole.
If this is not true, can someone explain why?

Thanks,
Helix_angle
 
  • #4
Helix_angle,
if this were to happen it would mean that two observers might disagree about what they are seeing, one saying BH the other saying it's a normal mass. The apparent increase in mass due to relative velocity does not increase the perceived gravitational pull. Ignoring black holes, it would mean that one observer might see tall buildings collapse under their own weight and another observer seeing them standing.

I can't prove it but I would say nature rules out such chaos.

M
 
  • #5
Ok, I think I mixed-up SR and GR -- because your question seems to. Recession velocity due to the expansion of the universe (a consequence of GR) has no associated special relativistic effects like mass increase. It isn't a "real" speed - it just looks like objects are moving because the space between them is increasing.

Now on the related question of whether you could give an object enough energy to turn it into a black hole, I'm not so sure -- someone with a deeper understanding of SR and GR might be able to take that.
 
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  • #6
ah - of course. The recession due to spacetime expansion is not a relitavistic speed as I was imagining it. This makes sense.
I'd be interested if someone has an answer to the black hole question though. It was mentioned that they may be creating 'mini black holes' in the soon to be online LHC. I wonder if these are caused simply by the enormous velocity of the accelerated particles as I described above, or something to do with the energy involved in the collision?


Thanks for your help,
Helix_Angle
 
  • #7
helix_angle said:
you didn't read my question properly. I was asking whether general relativity provides that at some point approaching the speed of light the mass an object relative to an observer must reach the point where photons reflected from its surface can no longer escape its mass, causing it to appear to the observer to be a black hole.
If this is not true, can someone explain why?

Thanks,
Helix_angle


Imagine a planet with about the the same size and mass of the Earth is whizzing past you at a relativistic velocity such the clocks on that planet are slowed down by a factor of 2 by time dilation. On Earth a object dropped from a height of about 10 meters takes about one second to hit the floor. A person standing on the top of the planet dropping a similar object from the same height would measure the time for the object to fall as half a second according to his clock if all else is equal. length contraction is not involved when we consider distance orthogonal to the motion. By his calculations the acceleration of gravity would be 4 times as fast as on the the Earth. now SR tells us the laws of physics are the same in all reference frames so the object must fall slower. That tells you that the gravitational effect is reduced, not increased by relative motion. The inertial mass of the object is increasing but not its gravitational mass. SR tells us that force perpendicular to the motion is reduced by gamma and this applies to gravity too. So the gravitational force acting on the object is halved and the inertial mass of the object has doubled. F=ma so a' =F'/m' = (f/2)/(m*2) = a/4 which agrees with the value I gave earlier. Hopefully the argument given here will convince you that while inertial mass can be viewed as increasing with relative motion it is not true that the gravitaional mass is increasing. In fact it is reducing.

So the answer to your last question about creating mini black holes in a collider is that they will be created by the energy of collisions rather than by apparent increase of relativistic mass.
 
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  • #8
helix_angle said:
I wonder if these are caused simply by the enormous velocity of the accelerated particles as I described above?
This question is answered in this FAQ, "http://www.weburbia.demon.co.uk/physics/black_fast.html" ".
 
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  • #9
Thanks Kev - that explains things very well.
Cheers,
Helix_Angle
 

1. Why are there fewer visible stars in far away galaxies?

There are a few reasons for this. One is that the light from these stars has to travel a very long distance to reach us, and some of it gets absorbed or scattered along the way. Additionally, the farther away a galaxy is, the more its light is redshifted due to the expansion of the universe, making the stars appear dimmer. Finally, the number of stars we can see in a galaxy depends on its size and age, so galaxies that are farther away may simply have fewer stars.

2. Can we see all the stars in a far away galaxy?

No, we cannot. The amount of light that reaches us from a far away galaxy is limited by the size and brightness of the stars, as well as any intervening dust or gas. Additionally, the resolution of our telescopes is limited, so we may not be able to see individual stars even if they are present in the galaxy.

3. Are there any other factors besides distance that affect the visibility of stars in far away galaxies?

Yes, there are. The age and size of the galaxy, as well as the amount of dust and gas present, can also affect the visibility of stars. Galaxies that are very old or small may have fewer stars, while those with a lot of dust and gas may have their stars obscured from our view.

4. Can we use technology to see more stars in far away galaxies?

Yes, advancements in technology have allowed us to see more stars in far away galaxies than ever before. For example, the Hubble Space Telescope has a much larger aperture and can capture more light, allowing us to see fainter stars. Also, new techniques such as adaptive optics can correct for distortions caused by Earth's atmosphere, allowing for clearer images of distant galaxies.

5. Are there any limitations to how far away we can see stars in galaxies?

Yes, there are limitations. As we look further and further into the universe, the light from galaxies becomes more and more redshifted, making it more difficult to detect individual stars. Additionally, there may be galaxies that are so far away that their light has not had enough time to reach us since the beginning of the universe. Thus, there is a limit to how far back in time we can see stars in distant galaxies.

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