derek101 said:
If the balloon analogy is a good analogy,I have a question,because the galaxies are expanding away from each other,what is the fastest galaxy that we know to be traveling away from us,and how far can we see around to the other side of the balloon?
I like your question, except I think it's a bad idea to talk of galaxies "traveling away from us", or to think of them as doing that.
In a uniform pattern of distance expansion nobody is traveling in the usual sense because
nobody gets anywhere.
It is not motion. It is a change in geometry.
That's a big reason WHY the balloon analogy has generally been helpful to the people who have actually gone and looked at the short movie. Google "wright balloon model"
The thing it does is it shows each galaxy staying fixed at the same latitude longitude place, while photons of light actually travel between and among them. The photons of light always travel at the same speed. You can check that by watching the movie.
And yet a photon of light even though you can see it traveling always at the same speed, does not necessarily get to its destination at that rate. The distance between it and where it is going can actually increase for a while (until the expansion rate slows).
It is a helpful model because you can learn a lot by watching carefully and you can learn a lot which SOUNDS paradoxical when said in words but is actually quite reasonable.
So I hope you have watched that movie or will do so before you start discussing the balloon analogy here.
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In direct answer to your questions. We can see the light from matter that is NOW 45.5 billion LY from us. It didn't use to be so far away when it emitted the light which we are not getting from it. But NOW the matter we are looking at, the farthest, is 45.5 billion LY from here, so that is how far we can see.
I am using the definition of distance called proper distance which means what you would measure by conventional means like radar or a long string, if you could just stop the expansion process NOW to give yourself time to measure.
The latest NASA estimate of the circumference of the U, the MINIMUM circumf that it could be now, if it is finite at all, is about 600 billion LY. (Again proper distance)
You asked how far we can see and is that around to the other side and the answer is no it is not around to the other side, the 45 is only a little ways compared with the 600.
And the 600 is only a minimum, a lower bound estimate. It might be much bigger. They did not give any estimate of upper bound.
You asked what rate the distance to the most distant galaxy (so far) is increasing. I believe it is about 2.3 times c. we see other more distant stuff, that is receding at 3 times c. But that stuff has not cooled and condensed into galaxies yet. If you have further questions I hope you will start a thread and ask them. The most distant galaxy is, I believe, UDFj-39546284
If you google it you find that the estimated redshift is 10.3.
Then follow the "morgans" link in my sig to morgan's calculator. Or simply google "cosmos calculator".
Put in the 3 standard parameters (.27 for matter, .73 for cosmo constant, 71 for Hubble rate) and then put in 10.3 and press calculate. It will tell you the current distance and the current rate that distance is increasing which is 2.3c.