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.