Expanding universe and age of light

Click For Summary

Discussion Overview

The discussion centers on the concepts of the expanding universe and the implications of redshift in relation to the age of light from distant galaxies. Participants explore the nature of cosmic expansion, the interpretation of redshift, and the relationship between the distance of galaxies and their observed light, touching on theoretical and conceptual aspects of cosmology.

Discussion Character

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

Main Points Raised

  • Some participants suggest that the redshift of galaxies indicates they are moving away, while others clarify that the expansion of the universe is about space itself growing rather than galaxies moving through space.
  • There is a discussion about whether the age of light affects the interpretation of redshift, with some arguing that it does not matter because the redshift is a result of the stretching of space.
  • Participants express confusion about the nature of space and whether objects are actually getting larger or if the space between them is expanding.
  • Some participants propose that the redshift observed today reflects the historical expansion of the universe, with light taking time to reach us, thus representing conditions from the past.
  • There is mention of the acceleration of the universe's expansion, with some arguing that terminology like "space is expanding" may be misleading.
  • Questions arise regarding whether the observed redshift corresponds to current speeds of galaxies or their speeds from millions of years ago.
  • Some participants note that mutual gravitational forces can affect the movement of galaxies within clusters, complicating the overall picture of cosmic expansion.

Areas of Agreement / Disagreement

Participants generally agree that the redshift indicates a historical perspective on the universe's expansion, but multiple competing views remain regarding the interpretation of redshift, the nature of space, and the implications of cosmic expansion. The discussion remains unresolved with respect to some of these conceptual clarifications.

Contextual Notes

There are limitations in the discussion regarding the definitions of space and movement in the context of general relativity, as well as the complexities of interpreting redshift data over time.

deuspisi
Messages
7
Reaction score
0
OK I might be stupid and english isn't my native language, so I'm sorry in advance.
So:
The red shift is bigger, the further away a galaxy is (they move away faster), and the closer it is, the shift is smaller and it goes to blue for Andromeda (towards). Everyone knows that.
BUT
When you consider that the light from the far galaxy is very very old, and from the close galaxy is new, don't you think that the universe WAS expanding long time ago and now it's collapsing?
It's so simple I can't believe i might be right. I must be wrong. Please tell me where i go wrong...
 
Space news on Phys.org
It is not what you describe. The expansion is about space itself growing and not really about the galaxies "moving". The redshift is not really a Doppler shift but an effect of space (and therefore the light wavelength) stretching out.

To add to this, the galaxies also do move, but generally in random directions. This causes an additional Doppler effect which when a galaxy moves towards us can give a net blueshift. You have to take all effects into account properly.
 
  • Like
Likes   Reactions: deuspisi
Orodruin said:
It is not what you describe. The expansion is about space itself growing and not really about the galaxies "moving". The redshift is not really a Doppler shift but an effect of space (and therefore the light wavelength) stretching out.

To add to this, the galaxies also do move, but generally in random directions. This causes an additional Doppler effect which when a galaxy moves towards us can give a net blueshift. You have to take all effects into account properly.

Well I'm a little confused right now. What exactly is "space" then (if not the distance between two things). Am I getting bigger right now, my molecules and atoms, or is the space between them getting bigger? And relative to what?
 
deuspisi said:
Well I'm a little confused right now.
You should be, these are really not concepts which let themselves be well explained with words.

deuspisi said:
What exactly is "space" then (if not the distance between two things).
Space is generally a part of space-time. It describes a background in which physics occur. A measure of space is distance, but it is possible for this distance to increase without two objects "moving" with respect to each other. I say moving with quotations because in general relativity this requires some additional definitions if the objects are not at the same place.

If you have not seen the balloon analogy, I recommend you look it up (and remember that "moving" means moving relative to the rubber in the balloon, which represents space).

deuspisi said:
Am I getting bigger right now, my molecules and atoms, or is the space between them getting bigger? And relative to what?
No, you are not getting bigger. The forces involved in holding you together are far stronger than the expansion could overcome.
 
  • Like
Likes   Reactions: deuspisi
First I want to thank you for responding. I was looking for answer for months but somehow didn't get the right article to read.
I know the balloon analogy, but I thought it was simle Doppler, therefore my question about the age of the red shift. Now I know it is cosmological redshift (thank you), and the space universally is stretching the wavelength, not the movement, therefore the age of light doesn't matter.
One more question: In that case, (if the space is constantly stretching) is this a constant shift (same speed), or moving toward red/blue (accelerating/decelerating) for far and near galaxies. I can't find any information. If you have links, please share. Thank you again.
 
The redshift affects all light in the same way regardless of the source. The factor with which the wavelength changes is simply the scale factor today divided by the scale factor at the time the light was emitted. In some sense, it just compares the size of the universe at the different times.
 
  • Like
Likes   Reactions: deuspisi
Orodruin said:
The redshift affects all light in the same way regardless of the source. The factor with which the wavelength changes is simply the scale factor today divided by the scale factor at the time the light was emitted. In some sense, it just compares the size of the universe at the different times.
I understand that.
But if the wavelength (red shift) of all galaxies changes over time (from the past 10 years readings for example) toward red/blue, that means space expanding speed is changed, right?
 
deuspisi said:
I understand that.
But if the wavelength (red shift) of all galaxies changes over time (from the past 10 years readings for example) toward red/blue, that means space expanding speed is changed, right?
This whole "space is expanding" is really not good terminology (yes, I know you see it EVERYWHERE in pop science). Things just get farther apart, and yes, they are getting farther apart ever faster. That's what it means that the recession is accelerating
 
  • Like
Likes   Reactions: deuspisi
phinds said:
This whole "space is expanding" is really not good terminology (yes, I know you see it EVERYWHERE in pop science). Things just get farther apart, and yes, they are getting farther apart ever faster. That's what it means that the recession is accelerating

So when we observe galaxy 100 mil ly away with some speed (red shift) is this the current speed of the galaxy, or the speed 100 mil years from the past?
 
  • #10
deuspisi said:
So when we observe galaxy 100 mil ly away with some speed (red shift) is this the current speed of the galaxy, or the speed 100 mil years from the past?
We see things as they were in the past. We also have enough information, having observed LOTS of galactic recessions, to have a good idea what it's doing "now". I put now in quotes 'cause that's a bit of a tricky subject.

This is how we know that the observable universe is about 13+ Billion years old and yet the observable universes has a radius "now" of about 50 Billion light years.
 
  • Like
Likes   Reactions: deuspisi
  • #11
Thank you, people.
Sorry if i annoyed you with my ignorance.
I have more questions about how the expansion is stretching the wavelength, but I'll read more (now i know where).
bb
 
  • #12
deuspisi said:
Thank you, people.
Sorry if i annoyed you with my ignorance.
I have more questions about how the expansion is stretching the wavelength, but I'll read more (now i know where).
bb
Hey, that's what we're here for. Glad to see you are learning this stuff. :smile:
 
  • Like
Likes   Reactions: deuspisi
  • #13
deuspisi said:
Well I'm a little confused right now. What exactly is "space" then (if not the distance between two things). Am I getting bigger right now, my molecules and atoms, or is the space between them getting bigger? And relative to what?
The average distance between galaxies is getting larger over time. There are some galaxies that are close to one another that are locked in their mutual gravitational attraction (such as the Milky Way and Andromeda), but most galaxies are moving away from one another in a pretty uniform fashion (so that a galaxy that is twice as far away is, on average, receding at twice the speed).
 
  • #14
The mutual gravitation seems to hold for clusters of galaxies and maybe superclusters.
 
  • #15
mathman said:
The mutual gravitation seems to hold for clusters of galaxies and maybe superclusters.
my original question was "the red shift that we see today: is it old (outdated) data from millions years ago?" because light need time to get to us, and what we see now is actually what was long time ago. that's all I'm asking.
 
  • #16
deuspisi said:
my original question was "the red shift that we see today: is it old (outdated) data from millions years ago?" because light need time to get to us, and what we see now is actually what was long time ago. that's all I'm asking.
Yes, this is true. So when we look far away, we see the expansion history of the universe. The rate of expansion has been slowing over the last few billion years, and it appears to be approaching a constant expansion rate (given by the cosmological constant).
 
  • #17
Chalnoth said:
Yes, this is true. So when we look far away, we see the expansion history of the universe. The rate of expansion has been slowing over the last few billion years, and it appears to be approaching a constant expansion rate (given by the cosmological constant).
That's a very confusing way to express it to a noobie. The rate of the ACCELERATION is slowing to a constant but since the recession is still accelerating and will continue to accelerate, the expansion is getting faster and faster and will continue to get faster still.
 
  • #18
phinds said:
That's a very confusing way to express it to a noobie. The rate of the ACCELERATION is slowing to a constant but since the recession is still accelerating and will continue to accelerate, the expansion is getting faster and faster and will continue to get faster still.
IMO, this is even more confusing. I thought that we have agreed some time ago (will have to look it up) that the (fractional or %) expansion rate is represented by H(t) and that it is dropping to a constant value. The other value is the recession rate of specific galaxies and it is increasing today and in the future due the constant H.
 
  • #19
Chalnoth said:
Yes, this is true.
I believe this is confusing based on what the OP wrote earlier. While it is true that you can infer the expansion history, it is not true that seeing further objects redder implies that they were going away faster.
 
  • #20
Jorrie said:
IMO, this is even more confusing. I thought that we have agreed some time ago (will have to look it up) that the (fractional or %) expansion rate is represented by H(t) and that it is dropping to a constant value. The other value is the recession rate of specific galaxies and it is increasing today and in the future due the constant H.
Yes, but I'm talking about how it looks to a noobie who doesn't yet understand those terms.
 
  • #21
Orodruin said:
I believe this is confusing based on what the OP wrote earlier. While it is true that you can infer the expansion history, it is not true that seeing further objects redder implies that they were going away faster.
My yes in that statement was solely in response to the quoted question about whether the light we see is outdated. It is.
 
  • #22
Chalnoth said:
My yes in that statement was solely in response to the quoted question about whether the light we see is outdated. It is.
I understand that, but based on the inference the OP made from this fact, I just wanted to make it clear that that inference was not correct.
 

Similar threads

  • · Replies 5 ·
Replies
5
Views
4K
  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 2 ·
Replies
2
Views
1K
  • · Replies 8 ·
Replies
8
Views
3K
  • · Replies 23 ·
Replies
23
Views
4K
  • · Replies 18 ·
Replies
18
Views
3K
  • · Replies 39 ·
2
Replies
39
Views
8K
  • · Replies 19 ·
Replies
19
Views
5K
  • · Replies 7 ·
Replies
7
Views
4K
  • · Replies 16 ·
Replies
16
Views
3K