Viewing a far away galaxy through a wormhole

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SUMMARY

This discussion explores the hypothetical observation of two galaxies, A and B, located billions of light years away, with galaxy A viewed through a wormhole. The redshift observed in galaxy A can vary significantly based on the motion of the wormhole's mouths, potentially resulting in extreme red, zero, or blue shifts. In contrast, galaxy B, viewed through normal space, would exhibit the standard Hubble redshift. The characteristics of the wormhole, including its curvature and the motion of its mouths, play a crucial role in determining the observed frequency shift of light from galaxy A.

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  • Understanding of redshift and its implications in astrophysics
  • Familiarity with the concept of wormholes in theoretical physics
  • Knowledge of Hubble's Law and its application to distant galaxies
  • Basic principles of light frequency and Doppler effect
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  • Research the effects of wormhole geometry on light propagation
  • Study the implications of redshift in cosmology and galaxy formation
  • Explore the theoretical models of wormholes and their characteristics
  • Examine the Doppler effect and its relevance to astrophysical observations
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Astronomers, astrophysicists, and students of theoretical physics interested in the implications of wormholes and redshift in cosmic observations.

NWH
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Hypothetically speaking of course, if we were to observe a galaxy billions of light years away on the opposite end of the universe through a wormhole, what would the red shift look like compared to other galaxies in the observable universe? For example, I'll set up a thought experiment.

We have two galaxies, galaxy A and galaxy B. Both galaxies are at the same distance away in the the farthest reaches of the observable universe, both have the exact same brightness and both are traveling at the exact same velocity. Galaxy A is on the left, galaxy B is on the right, however in front of galaxy A we have an open wormhole like a looking glass giving us a closer look at that galaxy. What would we see in the red shift? How would the red shift differ between galaxy A and galaxy B?
 
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NWH said:
Hypothetically speaking of course, if we were to observe a galaxy billions of light years away on the opposite end of the universe through a wormhole, what would the red shift look like compared to other galaxies in the observable universe? For example, I'll set up a thought experiment.

We have two galaxies, galaxy A and galaxy B. Both galaxies are at the same distance away in the the farthest reaches of the observable universe, both have the exact same brightness and both are traveling at the exact same velocity. Galaxy A is on the left, galaxy B is on the right, however in front of galaxy A we have an open wormhole like a looking glass giving us a closer look at that galaxy. What would we see in the red shift? How would the red shift differ between galaxy A and galaxy B?

It depends on what kind of wormhole you are thinking about. Redshift is caused by space curving along the light beam, so in principle you would see less redshift. However you have to remember that wormholes are crazy curved themselves, so all bets are off unless you give me the precise form of it.
 
NWH said:
How would the red shift differ between galaxy A [viewed though a wormhole] and galaxy B [viewed through normal space]?
Bracketed insertions mine.

The frequency shift of light from galaxy A could range from being extremely red, to zero, to extremely blue. It depends on the motion of the wormhole mouths. A course, light from galaxy B would have the usual Hubble redshift.

Suppose that the wormhole mouth near Earth is approximately stationary relative to Earth. Then the frequency shift depends on the motion of the far mouth (the one nearer to galaxy A) relative to galaxy A.

If the far mouth is receding from galaxy A: redshift
If the far mouth is stationary relative to galaxy A: no frequency shift.
If the far mouth is approaching galaxy A: blue shift.

This ignores any frequency shifts due the wormhole's gravity, which would depend on the particular characteristics of the wormhole.
 

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