SteveCNC":1acu76y7 said:
One thing that bothers me about the acceleration of expansion is that that farther we look (distance/time) we see things moving faster away than closer objects . So what is it moving faster anyway , is it us (our galaxy) or them (the observed galaxy) ? If it's the observed galaxy , are we not looking way back in time so what we see is light emited over a billion years ago , so doesn't that mean that it was moving that fast a long time ago ?
It can get confusing, can't it? Especially as there are 2 different concepts involved, concerning the "speed" at which distant galaxies are, or were, receding. As we look back past 5 or 6 billion years ago we are looking at the universe when it was still decelerating, so the further we look, the faster a galaxy was apparently receding.
But it is not the acceleration of the expansion that causes apparent recession speed to increase with distance, it is the expansion itself, whether it accelerates or decelerates. At any given time, the whole universe is thought to be expanding at the same rate, but that rate changes, over time.
So at any given time, the further away an object is, the faster it would be receding, as the expansion means all distances scale up by the same factor. If 1 billion light-years becomes 2, then 10 billion light-years becomes 20! That is the principle around which we model the expansion of the universe, built using the slice of the history of the universe we can see.
With distant galaxies, their redshift tells us how much the universe has expanded since the light we are seeing was originally emitted.
If we work out how far away those galaxies were when they emitted that light
(by apparent size, dimness, or proximity to something we already know the distance of, for instance), we can work out how fast they were apparently receding at that time, assuming everything we see began in the same place.
If we multiply that distance by the amount the universe has expanded
since (using their redshift), we can work out how far away they would be today, and thus how fast they would have had to apparently recede to get there.
I say "apparently" recede, as they are not actually moving much relative to the space around them, it is the space between them and us that
apparently expands! This has always been happening all over the universe , meaning that the further away something is, the faster it is being "moved away" by the expansion of the universe.
So when we extrapolate how the universe would be today (13.7 billion years old, 46 billion light years in radius), the further away (in distance) we "look", the faster something
is receding. And when we look at the slice of the history of the universe we can actually see, the whole range of expansion rates is played out before us, with the closer objects seen as they were whilst the universe has been accelerating, and more distant objects seen as they were when the universe was decelerating, so the further we look, the faster something
was receding.
Or something like that..