Distant stars and length contraction

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Discussion Overview

The discussion revolves around the implications of length contraction and stellar aberration for determining Earth's motion relative to the universe. Participants explore whether the distribution of stars observed from different frames can indicate whether Earth is moving and how this relates to concepts like the Hubble flow and the cosmic microwave background (CMB) frame.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • Some participants propose that a stationary observer sees stars uniformly, while a moving observer would see a concentration of stars due to length contraction.
  • Others argue that the effect of stellar aberration alters the visual perception of star distribution, leading to a concentration of stars ahead of the observer.
  • A later reply introduces the concept of the Hubble flow, suggesting that if the distribution of nearby galaxies appears isotropic, the observer is at rest relative to them.
  • Participants discuss the significance of the CMB frame, with some suggesting it may yield interesting symmetries or signatures, while others question the physical basis for considering it a preferred frame.
  • Some express that the existence of the CMB frame does not imply it is physically special, contrasting it with other frames that may not have the same significance.
  • There are mentions of the limitations of using the CMB frame for discussions about motion, emphasizing the need for qualifiers when stating motion relative to it.
  • Some participants highlight that isotropy of matter distribution is a boundary condition rather than a fundamental law of nature.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the implications of the CMB frame and the nature of motion relative to the universe. There is no consensus on whether the CMB frame is special or how it should be interpreted in the context of special relativity.

Contextual Notes

Participants acknowledge the complexity of defining motion and the implications of different frames of reference, particularly in relation to the isotropy of space and the laws of nature. There are unresolved questions about the significance of the CMB frame and its relationship to other frames.

Ookke
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Please see the picture. Red dots are stars, lines are the path that light takes, our observer is at center. Assuming that stars are somewhat uniformly spread around us, I suppose that stationary observer (left picture) sees about as many stars in every direction, but an observer moving in y-direction (right picture) sees stars concentrated on the sides due to length contraction and fewer stars up and down. Can we use this method to tell is Earth moving relative to rest of the universe? If space looks same in every direction, we are not moving?
stars.png
 
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Ookke said:
Assuming that stars are somewhat uniformly spread around us,
You are also assuming a finite amount of stars, and nothing beyond them.

Ookke said:
but an observer moving in y-direction (right picture) sees stars concentrated on the sides due to length contraction and fewer stars up and down.
Not quite:
https://en.wikipedia.org/wiki/Aberration_of_light

Ookke said:
Can we use this method to tell is Earth moving relative to rest of the universe?
Relative to some stars in the universe.
 
Ookke said:
Can we use this method to tell is Earth moving relative to rest of the universe? If space looks same in every direction, we are not moving?

This is one way of defining the Hubble flow. If the distribution of nearby galaxies looks isotropic and homogeneous, you're at rest relative to the average motion of the nearby galaxies. We then say that you're at rest relative to the Hubble flow.

An equivalent method is to look for the frame in which the CMB looks isotropic.
 
In addition to the aberration mentioned by AT there is also Doppler shift. This is maybe not so relevant for stars as for the CMB.
 
I don't think your question is really answered. What you describe is a way to determine your motion with respect to a bunch of stars. There's no problem with this. But the other part of your argument, that there is something special about the frame where these stars at rest, is not established. Indeed, in SR, there's nothing special about it, the frame where the CMB is at rest, or the frame where Lincoln was shot. These frames may be interesting to us, but they are not physically special.
 
Vanadium 50 said:
I don't think your question is really answered. What you describe is a way to determine your motion with respect to a bunch of stars. There's no problem with this. But the other part of your argument, that there is something special about the frame where these stars at rest, is not established. Indeed, in SR, there's nothing special about it, the frame where the CMB is at rest, or the frame where Lincoln was shot. These frames may be interesting to us, but they are not physically special.

The frame where CMB is at rest might yield other interesting symmetries or signatures.
 
Something that should be clarified. As AT mentioned, the effect of stellar aberration means that what you'd visually see through a telescope would be different than your diagram, you'd "see" the stars concentrated ahead of you. There's some pictures at http://www.exo.net/~pauld/stars/PD_images_relativ.html, these were probably taken from the paper "In search of the starbow", http://scitation.aip.org/content/aapt/journal/ajp/47/4/10.1119/1.11834. This paper used to be online but I don't see it anywhere anymore.

The image you drew can be described as what you'd compute from your photographs, using the concept of "now" applicable to your frame of reference and compensating for travel time.

It is true that there is a special frame of reference in which the universe, as a whole, is isotropic (the same in all directions). This is usually called the cosmic microwave background frame or CMB frame, people replace the distribution of stars (in your picture) with measurements of the background microwave radiation from the big big bang, as in the WMAP experimenmts http://map.gsfc.nasa.gov/.

However, it would be confusing at the minimum (and generally regarded as wrong) to assume that people were using this particlaur frame in any given instance. There's nothing that forces us to use this frame, and many times it's inconvenient. So when you want people to know you're using that frame, you can specify "the CMB frame", and people will known what you're talking about (well, physicists and astronomers at least.

In short, the existence of the CMB frame doesn't really excuse sloppiness in descriptions of motion. It's OK to say "not moving with respect to the CMB frame", it's ambiguous at the minimum to say "not moving" without the necessary qualifiers as "compared to what".
 
1977ub said:
The frame where CMB is at rest might yield other interesting symmetries or signatures.

Why? How is this different from the frame where Lincoln was shot? "One sounds plausible and the other sounds crazy" is not a good answer - how physically do they differ and what is the mechanism for this to be a preferred frame?
 
Vanadium 50 said:
1977ub said:
The frame where CMB is at rest might yield other interesting symmetries or signatures.
Why? How is this different from the frame where Lincoln was shot? "One sounds plausible and the other sounds crazy" is not a good answer - how physically do they differ and what is the mechanism for this to be a preferred frame?

Examples of symmetries: (1) matter is homogeneous and isotropic, (2) CMB is isotropic on the average (dipole moment vanishes).

Examples of conveniences: (1) stress-energy tensor has a simple form, (2) observations made on Earth can be discussed without boosting, (3) energies of cosmic rays correspond to the energy scale of the processes that created them.
 
  • #10
bcrowell said:
Examples of symmetrie

But these are symmetries of the environment one is in. Not the sort of thing you would think would overthrow SR - which is what this would encounter.
 
  • #11
pervect said:
This is nice. Not exactly what I thought, but there is some concentration of stars and the rear view gets empty. At least we can rule out the possibility that Earth is moving very fast relative to the stars we see?

CMB frame that was brought up sounds like preferred frame to me, at least for aesthetic reasons. SR states that laws of nature must be the same in every inertial frame. If we consider "space is isotropic" as law of nature, then CMB frame would be the only valid one, but this would be very strict position. It sounds plausible that CMB frame could have some difference in gravitational or even inertial effects compared to other frames, but "sounds plausible" of course has no value by itself.
 
  • #12
Vanadium 50 said:
But these are symmetries of the environment one is in. Not the sort of thing you would think would overthrow SR - which is what this would encounter.

Maybe we had different understandings of what the OP was talking about. I didn't interpret this thread as being about overthrowing SR.
 
  • #13
bcrowell said:
I didn't interpret this thread as being about overthrowing SR.
And I didn't mean it that way. It's always about limits of applicability too, but overthrowing SR altogether is not reasonable to even try. CMB frame is interesting, though.
 
  • #14
Ookke said:
CMB frame that was brought up sounds like preferred frame to me, at least for aesthetic reasons. SR states that laws of nature must be the same in every inertial frame. If we consider "space is isotropic" as law of nature,
Isotropy of the distribution of matter is a boundary condition, not a law of nature. Thread closed.
 

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