0 |
| G G G
3,5 bly M..1..2..3
| x
| x G G G
8,5 bly M .x. 1 . . 2 . . 3
| x
|x G G G
13,5 bly M . . 1 . . 2 . . 3
time
- The above figure shows the 3 balloons at 10 billion lightyears (bly) ago, at 5 bly ago and at the present.
- At each epoch there are 4 Galaxies shown: M (Milky way), G1, G2 and G3
- Galaxy G2 at the 3,5 bly line is a special one. The distance to "M" is 10 bly and we can currently see this young Galaxy. The light path from that Galaxy towards "M" are the letters "x".
- Galaxy G3 we could see at a younger age/stage as G2 and Galaxy G1 we will see at an older age/stage as G1
- The problem with the picture is how can we see G2 at a distance of 10 bly, while the age of the Universe is only 3,5 bly ?
- The above picture shows cosmic expansion. This expansion is homogeneous.
- The above picture also shows that the expansion is accelerating. A major question is how do we know that the Universe is accelerating. Based on which data.