Expansion of space and looking back in time

In summary: We are at the center, of course, from our point of view, but so is any other point in the universe. The universe is infinite and expanding, and the expansion is uniform. So, from any point in the universe, it looks like it is expanding away from you, just as the surface of the balloon expands away from any point on it. There's an old saying that the universe is like a large ball, expanding as it cools down from the Big Bang. But that's not right, because the ball has a center, and the universe doesn't. The universe is more like the surface of a balloon as it expands, but the balloon has a center, and the universe doesn't.
  • #1
DARKSYDE
50
0
when we observe objects that are billions of lights years away are we also observing the expanse of space as it existed then? let's say 10 billion light years ago. could we call it a compressed universe as opposed to the expanded universe we are in now and observing from

the universe would have only been 3.7 billion light years "big" (estimate base on current observations). it seems odd that we could look back at our universe when it was smaller yet we are still in it.
 
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  • #2
DARKSYDE said:
... it seems odd that we could look back at our universe when it was smaller yet we are still in it.


Good question that have also puzzled me. The key to understanding is the expansion of curved spacetime.


Observable Universe
First, when talking about how "big" the universe is/was – we must remember to emphasize that it’s the observable universe we are talking about. The whole universe might be infinite, we just don’t know yet. Some scientist’s claims that there is proof of a universe a least a thousand times bigger than the observable universe, and most agrees that the observable universe is 93 billion light-years in diameter.


Expansion of Curved Spacetime
This is quite complicated things involving the General Theory of Relativity. However, it can be understood by a layman on a basic level, omitting two dimensions of space, and focusing on one dimension of space and one of time.

The picture below shows how a light ray (red line) can travel an effective distance of 28 billion light years (orange line) in just 13 billion years. This also reveals the fact that observable universe = calculated visible universe.

250px-Embedded_LambdaCDM_geometry.png


For more info, read http://en.wikipedia.org/wiki/Expanding_universe#Understanding_the_expansion_of_space" on Wikipedia.


Looking Back at the Universe
What are we looking at? Well, everything that we see when looking 'back' is right here and now. The photon hitting the camera or the eye is right here, and not 'there'. Confusing? Actually it turns out to be even more 'odd'...

You refer to objects when the universe was 3.7 billion years old. The fact is that we can photograph the whole (observable) universe when it was only 400 000 years old! And it looks like this:

080997_5yrFullSky_WMAP_512B.png


This 'baby-picture' of the universe shows the Cosmic Microwave Background (CMB) radiation (the oldest light in the universe) and is produced by The Wilkinson Microwave Anisotropy Probe (WMAP).

More info at http://map.gsfc.nasa.gov/" .

Here’s a schematic picture of the history of the universe, showing CMB at 400 000 years:

600px-CMB_Timeline75.jpg


How is this possible!? :confused:


Get Serious
Well, now it’s time to get real serious and look at the basic mechanism:

1) Photons always travel at the speed of light relative to the galaxies near them.

2) As the universe gets older, the galaxies do not expand, but the distance between the galaxies gets larger.

[PLAIN]http://www.astro.ucla.edu/~wright/cphotons.gif[/INDENT][/URL]

The animation shows the expansion of space and the evolution of the galaxy density, positions and the photon positions within a '78 billion light year box'. Each black dot represents a galaxy, and the two green dots are galaxies emitting red photons.

http://www.astro.ucla.edu/~wright/intro.html" made this excellent animation, and you’ll find a lot more of useful info at his Home Page:

http://www.astro.ucla.edu/~wright/photons_outrun.html"

Good luck!​
 
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  • #3
wow, just wow! thank you for the super informative reply. the resources you supplied should be a great read when i get home. thanks for your time.
 
  • #4
DARKSYDE said:
wow, just wow!

You’re welcome. Glad you found it useful. (I was also happy when I got this 'into my head' :smile:)
 
  • #5
btw the animation is great but it does seem to have a center... just saying
 
  • #6
DARKSYDE said:
... it does seem to have a center ...

It’s ok. The universe doesn’t have a center. Remove one dimension in space and think of it like the two-dimensional surface of earth. Where is the center on the surface of earth...??

(The answer is not Greenwich or the North Pole :wink:)

This is real hard to get into the head when thinking real space 3D, but this is how it is.

A lot more thoughts and answers about this in PF thread:
https://www.physicsforums.com/showthread.php?t=261161"
 
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  • #7
DARKSYDE said:
... center ...

I don’t know if this helps. But think of the 'baby-picture' of universe (CMB) applied on a sphere:

https://www.youtube.com/watch?v=<object width="425" height="344"><param name="movie" value="http://www.youtube.com/v/Aeq_pgirQ14&hl=en_US&fs=1&"></param><param name="allowFullScreen" value="true"></param><param name="allowscriptaccess" value="always"></param><embed src="http://www.youtube.com/v/Aeq_pgirQ14&hl=en_US&fs=1&" type="application/x-shockwave-flash" allowscriptaccess="always" allowfullscreen="true" width="425" height="344"></embed></object>

And then think of this sphere expanding (the white § are galaxies):

https://www.youtube.com/watch?v=<object width="425" height="344"><param name="movie" value="http://www.youtube.com/v/I9Cjxd4Mjog&hl=en_US&fs=1&"></param><param name="allowFullScreen" value="true"></param><param name="allowscriptaccess" value="always"></param><embed src="http://www.youtube.com/v/I9Cjxd4Mjog&hl=en_US&fs=1&" type="application/x-shockwave-flash" allowscriptaccess="always" allowfullscreen="true" width="425" height="344"></embed></object>
 
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  • #8
DARKSYDE said:
btw the animation is great but it does seem to have a center... just saying
It may sort of look that way, but if you moved anywhere in the animation, it would look exactly the same. Our universe is much like that, at least out to the limits of our vision.
 

Related to Expansion of space and looking back in time

1. How does the expansion of space affect our ability to see objects in the universe?

The expansion of space causes the light from distant objects to stretch, or redshift, which makes them appear to be moving away from us at faster speeds. This makes it more difficult to see these objects and their true distances.

2. How does looking back in time relate to the expansion of space?

As light travels through the expanding universe, its wavelengths get stretched, causing it to appear redder and indicating that it has been traveling for a longer period of time. This allows us to see objects as they were in the past, giving us a glimpse into the history of the universe.

3. Can we see all the way back to the beginning of the universe?

No, the expansion of space and the limitations of light speed prevent us from seeing all the way back to the beginning of the universe. The furthest we can currently see is the cosmic microwave background radiation, which is the earliest light that has reached us.

4. How do we know that the expansion of space is accelerating?

Through observations of distant supernovae, scientists have discovered that the expansion of space is not only continuing, but is also accelerating. This is thought to be due to the presence of dark energy, which is a mysterious force that counteracts gravity and pushes objects in the universe apart.

5. Is the expansion of space uniform throughout the universe?

No, the expansion of space is not uniform throughout the universe. It is influenced by the distribution of matter and energy, resulting in areas where space is expanding at a faster rate and others where it is expanding at a slower rate. This non-uniformity is known as the cosmic web.

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