If objects are accelerating, are we measuring the systems getting smaller?

Click For Summary

Discussion Overview

The discussion revolves around the implications of the universe's expansion on the visibility of distant objects, particularly whether accelerating objects are perceived as becoming smaller and dimmer over time. Participants explore observational tests and the significance of these changes in size and brightness, considering both theoretical and practical aspects of measurement.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants propose that as the universe expands, distant objects may become harder to see due to their increasing distance and speed, potentially leading to reduced brightness and apparent size.
  • Others question how significant these changes are, suggesting that on human time scales, the differences may be minuscule and not easily observable.
  • A participant presents a hypothetical scenario involving a galaxy moving away at a fraction of the speed of light, illustrating that the distance change over a short period is negligible compared to the vast distances involved.
  • Another participant challenges the notion that these changes are insignificant, arguing that if a nearby object were to move away, it would be noticeable, and questions why distant objects wouldn't exhibit similar detectable changes.
  • One participant cites the Hubble Law, noting that the change in distance over time is extremely small, making precise measurements impractical with current technology.
  • There is a suggestion that if measurements could achieve a high level of precision, it might be possible to observe the changes in brightness and size as proposed, but this remains impractical given current capabilities.

Areas of Agreement / Disagreement

Participants express differing views on the significance of the changes in size and brightness of distant objects due to the universe's expansion. While some acknowledge the theoretical possibility of detection, others emphasize the practical limitations and the minuscule nature of the changes involved, indicating that the discussion remains unresolved.

Contextual Notes

Limitations include the precision required for measuring distances to far-off galaxies, which is currently beyond available instruments and techniques. The discussion also highlights the vast scales involved, which contribute to the challenges of observation.

NWH
Messages
107
Reaction score
0
What the title implies, with the discovery that the universe is expanding, are we observing the systems becoming harder to see? You'd think that with the speed of the objects and the distances involved, things like brightness and actual size would be getting reduced...
 
Space news on Phys.org
What observational test would you propose to affirm that hyposthesis?
 
NWH said:
What the title implies, with the discovery that the universe is expanding, are we observing the systems becoming harder to see? You'd think that with the speed of the objects and the distances involved, things like brightness and actual size would be getting reduced...
Well, yes, but on human time scales, the differences are so miniscule as to be inconsequential.

Consider, for instance that we imagine that a galaxy that is one billion light years away is traveling at 0.1c away from us (this is just a number I pulled out of my backside...it's probably way, way wrong, so don't take it seriously).

Now, at this distance, if we wait for ten years, the galaxy will be a whole extra light year further away. One light year out of a billion. So sure, it's getting further away, and therefore dimmer and smaller. But it's just not going to be noticeable.
 
I find it hard to understand how the change is insignificant and can't be tested. Say for example, one of our planets fell out of orbit and started flying out of the solar system. We'd noticably see the object getting smaller and fainter, the further it got from the Earth. Now, if these distant objects are large enough and bright enough to be seen, and are accelerating away from us at such high speeds, why can't it be detected exactly?

If I take a picture of an apple, I can use the ammout of pixels in the image to determine it's apparent size in relation to another image of the same apple in which it is further away. Can't that same idea apply to this concept given that the image was at a high enough resolution to mark out noticable change?
 
NWH said:
I find it hard to understand how the change is insignificant and can't be tested..

The Hubble Law change in distance amounts to 1/140 of one percent every million years.

We can't measure distances to far-off galaxies with an accuracy of 1/140 of one percent, instruments and techniques are not even close to that level of precision.

But if we could determine distances to 1/140 of one percent, then your idea would work. We could just wait a million years and see if the distance changed (by brightness and size clues, just as you suggested!) But that is obviously impractical.

There are better ways to test Hubble Law expansion than what you propose (waiting for a measurable change in distance to show up). I hope you don't find this so hard to understand now. Your idea is impractical by a factor of about a million, to put it simply.
 
Last edited:
I see, thanks. It's hard to comprehend how insignificant it actually is, when we're talking about enormous bodies, at enormous distances and enormous speeds. You'd think you'd see at least something, puts into perspective just how BIG this universe is...
 

Similar threads

  • · Replies 23 ·
Replies
23
Views
4K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 134 ·
5
Replies
134
Views
12K
  • · Replies 37 ·
2
Replies
37
Views
6K
  • · Replies 24 ·
Replies
24
Views
3K
  • · Replies 24 ·
Replies
24
Views
3K