Expansion speed of the Universe

In summary, the evidence for an expanding universe comes from the observation of the redshift of distant objects, which is evidence of the universe expanding.
  • #1
discord73
29
0
if the farther a galaxy is from us the faster it is receding from us, and the closer a galaxy is to us the slower it is receding from us, and since the farther a galaxy is from us the further back in time we are seeing it, does that mean the universe is expanding slower now in the present and was expanding faster in the past?

Also is there a way of observing 2 other galaxies and being able to know or infer the rate at which the universe is expanding in relation to those two galaxies instead of just the rate at which the universe is expanding in relation to our galaxy and other galaxies?
 
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  • #2
Hi there,

Fact is that we do not live in a complete linear Universe. There are some galaxies close to the Milky Way, that do not move away from us. Just take our sister galaxy for example. Adnromeda will collide with the Milky Way in a little while. Therefore, it must be getting closer to us.

Cheers
 
  • #3
fatra2 said:
Hi there,

Fact is that we do not live in a complete linear Universe. There are some galaxies close to the Milky Way, that do not move away from us. Just take our sister galaxy for example. Adnromeda will collide with the Milky Way in a little while. Therefore, it must be getting closer to us.

Cheers

Yea, that's how galaxies collied, and how we have the local group and all that good stuff. I didn't think I implied in my post that we live in a linear universe
 
  • #4
I think you plot redshift (a measure of expansion between emission and observation) compared to distance (note: over cosmological distances, not just the local group), and find that, for example, a signal emitted 1bn years ago has more than half the redshift than a signal emitted exactly 2bn years ago, implying that the known amount of expansion occurs disproportionately in recent times.

Redshift is easy to find from standard candles and using luminosity distances, but I'm not sure how the distance itself is found (there are 4 parameters, redshift, distance, luminosity and observed intensity, and I can only see how 2 are observed)
 
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  • #5
MikeyW said:
but I'm not sure how the distance itself is found

Distance is determined by finding a standard candle, such as a super nova, in another galaxy then compareing it's known luminosity to it's apparent luminosity since light behaves by the inverse square law I believe, an object twice as far from us will appear 4 times fainter.
 
  • #6
That would be ok, but for the 1a supernovas which were used as evidence for accelerated expansion, the formula is modified to include the redshift for distances over which cosmic expansion is no longer negligible (eg. the light will be redshifted gravitationally, and as the universe expands, the density of photons falls, giving you a superficially low intensity).

The distance is (1+z) times closer than you would think in a universe that has expanded by redshift z between observation and emission.
 
  • #7
does that mean the universe is expanding slower now in the present and was expanding faster in the past?
you can't infer that from your statement.

Also is there a way of observing 2 other galaxies and being able to know or infer the rate at which the universe is expanding in relation to those two galaxies

There is nothing special about our Earth frame fo referenece...we are just another speck in the universe. It's believed the universe is homogeneous and isotropic so whether you make measurements and observations here or from a galaxy a billion light years away it is expected results will be the same.
 
  • #8
discord73 said:
if the farther a galaxy is from us the faster it is receding from us, and the closer a galaxy is to us the slower it is receding from us, and since the farther a galaxy is from us the further back in time we are seeing it, does that mean the universe is expanding slower now in the present and was expanding faster in the past?
Well, no what you've described is just simple expansion. To have an idea of how that expansion has changed over time, you have to look very carefully at how the relationship between speed and distance changes as you look further back into the past.

discord73 said:
Also is there a way of observing 2 other galaxies and being able to know or infer the rate at which the universe is expanding in relation to those two galaxies instead of just the rate at which the universe is expanding in relation to our galaxy and other galaxies?
Yes. It's just a simple coordinate transformation.
 
  • #9
Can someone explain in clear terms what the evidence is for an expanding universe? I think I may be close in my above post but don't think I understand where all the evidence comes from. I've tried reading the 1998 paper but it's more experimental than theoretical
 
  • #10
MikeyW said:
Can someone explain in clear terms what the evidence is for an expanding universe? I think I may be close in my above post but don't think I understand where all the evidence comes from. I've tried reading the 1998 paper but it's more experimental than theoretical
This essay may help:
http://www.talkorigins.org/faqs/astronomy/bigbang.html
 

Related to Expansion speed of the Universe

1. What is the expansion speed of the Universe?

The expansion speed of the Universe refers to the rate at which the Universe is expanding. It is measured in units of kilometers per second per megaparsec (km/s/Mpc). Currently, the expansion speed is estimated to be around 70 km/s/Mpc.

2. How is the expansion speed of the Universe measured?

The expansion speed of the Universe is measured using a variety of methods, including observing the redshift of distant galaxies, studying the cosmic microwave background radiation, and measuring the brightness of supernovae. These methods all provide different estimates, but they all point to an overall expansion rate of the Universe.

3. Has the expansion speed of the Universe always been the same?

No, the expansion speed of the Universe has not always been the same. In fact, it has been increasing over time. This is due to the presence of dark energy, a mysterious force that is causing the expansion of the Universe to accelerate. Scientists are still trying to understand the nature of dark energy and its effects on the expansion speed of the Universe.

4. How does the expansion speed of the Universe affect the formation of galaxies?

The expansion speed of the Universe plays a crucial role in the formation of galaxies. As the Universe expands, it cools down and becomes less dense. This allows matter to clump together and form galaxies. The faster the expansion speed, the more spread out the matter is and the longer it takes for galaxies to form.

5. Will the expansion speed of the Universe continue to increase?

Based on current observations, it is predicted that the expansion speed of the Universe will continue to increase. This means that the Universe will continue to expand at an even faster rate in the future. However, the exact rate and extent of this acceleration is still a subject of ongoing research and debate among scientists.

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