Universe expansion and hubble's law

In summary, the further a galaxy is from us, the faster it is moving away from us, accounting for an ever expanding universe.
  • #1
papa lazarou
4
0
I've been reading about the red-shift, the universe expanding, ect... And about the observation that the further a galaxy is from us, the faster it is moving away from us, accounting for an ever expanding universe.

I'm also curious about the fact that the further the galaxy, the further 'in the past' the observation of the state of the galaxy is.

Say a galaxy cluster is 500 million light years away from us, it is only telling us what the rate of expansion of the universe (in a broad sense) was 500 million years ago.

I'm sure that is accounted for when deducing the current rate of expansion of the universe, but I was wondering if the fact that galaxies far away move faster and accelerate faster is only because we observe them as they were closer to the origin of the universe.

So in term of a universe where the expansion is slowing down, it would make sense to see a closer, more 'up to date' galaxy be moving and expanding slower than a distant, 'younger' galaxy.

Or is that 'time-shift' effect due to observation and the speed of light insignificant compared to the actual 'red-shift' observed?
 
Space news on Phys.org
  • #2
It is not just the fact that the further a galaxy is, the greater its recession, that leads us to the conclusion that the universe will continue to expand. We would see that even if the universe's expansion was slowing. That conclusion is based on the exact ratio of red-shift to distance and how it changes over distances.

If we saw that this ratio did not change with distance, we could conclude that the rate at which the galaxy expands does not change over time. But we do not see this; what we see is that the red-shift/distance ratio varies with distance, which indicates that the universe expansion rate has sped up over time.
 
  • #3
thanks! :)

That conclusion is based on the exact ratio of red-shift to distance and how it changes over distances.

But does it changes over time? The red-shift we observe was some time in the past. Would it be fair to say that the red-shift of that galaxy 'now' could be different? Obviously we cannot observe that, since the speed of light is finite.

Maybe I need to read a bit more about the actual maths.
 
Last edited:
  • #4
I see what you are asking.
A galaxy that is 2 billion light years away exhibits a velocity that was happening 2 billion years ago and one that is 13 billion light years away is exhibiting the velocity it was traveling 13 billion years ago. We won't know what their present velocity is for another 13 billion years.

Has this been taken into account in the calculations and how?
 
  • #5
papa lazarou said:
thanks! :)
But does it changes over time? The red-shift we observe was some time in the past. Would it be fair to say that the red-shift of that galaxy 'now' could be different? Obviously we cannot observe that, since the speed of light is finite.

Maybe I need to read a bit more about the actual maths.

Papa,
for some hands-on experience with the conventional cosmo model, try this.google "cosmos calculator"

You first need to prime it by typing in the correct values of 3 parameters
Put in .27 for "matter fraction"
Put in .73 for "cosmological constant"
Put in 71 for Hubble.

Then you can put in any redshift and find out the recession speed THEN and the recession speed NOW!

this is the kind of thing I see you asking about. What the standard model says about the recession rate back then when it emitted the light, and the recession rate now on the day that we receive the light with our telescope.

All the numbers come from a simple math model called the Friedman equations. You can google Friedman or Friedmann with two Ns and get that to look at but it can actually help more to play around hands-on. The friedman model cosmos is built into the calculator.

there are a bunch of these calculators, all give you basically the same answers but some may give a lot more, with fancier terminology. Compare for example when you google
"wright calculator" or "cosmo calculator" (cosmo without the final S). You get more frills.
The first one I told you about is simpler to read because it is barebones. Doesn't give all the extras.

So why don't you google "cosmos calculator" and give it a try? Ask questions if you run into any difficulty or want to discuss the results.
 
  • #6
Cool. So it is taken into account.

Are galaxies really traveling that close to the speed of light from each other? That's amazing.

"*speed due to the expansion of space, not actual velocity.

ah.
 
Last edited:
  • #7
There was another logic flaw that was troubling me on the same subject, but seems to stem from my lack of understanding of cosmology and relativity.

I'm reading http://www.astro.princeton.edu/~aes/AST105/Readings/misconceptionsBigBang.pdf" first!
 
Last edited by a moderator:

1. What is the theory behind the expansion of the universe?

The theory of the expanding universe is based on the observation that galaxies are moving away from each other at an accelerating rate. This suggests that the universe is expanding, meaning that the space between galaxies is increasing over time.

2. How was Hubble's law discovered and what does it state?

Hubble's law was discovered by American astronomer Edwin Hubble in the 1920s. It states that the farther a galaxy is from Earth, the faster it appears to be moving away from us. This is represented by the equation v = H0d, where v is the galaxy's recessional velocity, d is its distance from Earth, and H0 is the Hubble constant which represents the rate of expansion of the universe.

3. What is the significance of Hubble's law?

Hubble's law is significant because it provides evidence for the expansion of the universe and supports the theory of the Big Bang. It also allows us to estimate the age of the universe and track its rate of expansion over time.

4. Is the expansion of the universe constant or is it changing?

The expansion of the universe is not constant, but rather it is accelerating. This was confirmed by observations of distant supernovae in the late 1990s, which showed that the expansion is actually increasing due to the presence of dark energy.

5. How does the expansion of the universe affect the future of our galaxy?

The expansion of the universe will continue to cause galaxies to move away from each other, eventually leading to the isolation of our own Milky Way galaxy. However, this process will take billions of years and will not have a significant impact on our daily lives. Additionally, the expansion may eventually lead to the "Big Rip," in which the universe expands so much that all matter is torn apart, but this is still a theoretical possibility and not a certainty.

Similar threads

Replies
6
Views
460
Replies
1
Views
1K
Replies
22
Views
1K
Replies
9
Views
1K
Replies
49
Views
3K
Replies
10
Views
155
  • Cosmology
Replies
11
Views
2K
Replies
2
Views
1K
Replies
19
Views
2K
Replies
9
Views
1K
Back
Top