Originally posted by: Chiropteran
The balloon analogy describes the motion of an expanding universe. I understand that. What I don't understand: where do they get the evidence that the universe is expanding?
See, you are putting the theory before the experimental data that proves the theory. It doesn't work like that, you need to have the data first to build the theory. The expanding balloon analogy is based on the assumption that galaxies further away from us are moving away from us faster. The problem I have is that how do we know they are moving away from us faster? All we know is that they were moving away from us faster when the light we now see was emitted.
For example, a galaxy "A" is 5 billion light years away and appears moving away from us faster than a galaxy "B" which is 2 billion light years away.
BUT, the light we see from galaxy "A" was actually emitted 5 billion years ago! I don't see how we can make any assumption about it's current acceleration based on how it was moving 5 billion years ago. What if it was just moving faster 5 billion years ago because it was still carrying momentum from the big bang, and has since slowed down? I don't see how we could know.
As I said above, a supernova far far away from us is *also* a supernova that occurred a long long time ago. With the information I have seen, it seems like the scientists just assume that the supernova is moving away from us faster because of the distance, while they ignore the possibility that it is moving away from us faster because it occurred a really long time ago and maybe things were moving faster back then.
Basically, I see it as a flawed experiment because there are two different variables- distance and time. How can they know the acceleration is due to distance but not time? I think it's impossible to tell. If all the galaxies were originally moving apart at some incredible speed, but they have been slowing down since the big bang, it would make perfect sense for us to perceive the furthest galaxies as moving faster, because we are seeing the light from them that occurred long ago before they had time to slow down.
We use redshift to determine the velocity that something is moving away from us at. This is the shift of spectral lines towards the red end of the spectrum similar to the doppler shift for sound. Hubble first noticed this and found that objects which were farther away were more redshifted than near objects. This redshift doesn't really come from the motion of the objects in question, but from the expansion of space.
If you emit a photon with a wavelength of 100nm, and space itself expands, the photon's wavelength expands as well, and you might now detect its wavelength to be 110nm.
So Hubble noticed this and came up with a relation for the expansion of the universe called the Hubble constant.
If you have a "standard candle" in the universe, some kind of event which you know is the same brightness no matter where it happens, then you can get an accurate plot of this expansion. From the luminosity (constant for standard candles) and the 1/r^2 dependence of detected flux (measured), you can deduce the distance to the object. You can then take a spectrum and calculate its redshift to find how fast it is moving away from you.
The standard candle is the supernova type 1a. If the Hubble constant is really constant, then plotting the redshifts of observed supernova as a function of distance should yield a straight line, the slope of which is the hubble constant. The Hubble telescope was commissioned with this as one of its major missions. What they found was the redshifts of these supernovae didn't follow a straight line, but a curve which indicated the distant supernovae were moving faster than expected.
This means that as the space between objects increases, so does the velocity with which they move apart. The acceleration of the universe isn't an acceleration that increases with time (although it does...) it's an acceleration that increases with distance (but because the objects are already moving away from each other, it also increases with time).