Okay, here's something I don't understand.
The Webb telescope will be able to pick up signals from the earliest time in the formation of the universe. Those signals have been traveling towards us for billions of years. That means we're billions of light-years away from the source of the signals. How, if we aren't traveling at the speed of light, has there been enough time for us to get so far away?
Or to put it another way, if those signals are traveling at the speed of light, how come they didn't pass us years ago? How come they're only just catching up with us now?
Assuming that the big bang and current standard model we are using at the moment, is more or less correct...
...currently our estimate for the size of the
observable universe is a sphere with a radius of about 46 billion light years around us. Which you will note is much bigger than 13.8 billion - which is roughly our estimate for the age of the universe. How can we see something 46 billion light years away if there has only been 13.8 billion years?
This disparity is caused by the expansion of the universe, which has been continually occurring since the start (very fast right at the start with inflation - a long bit of slower expansion afterwards - and, we currently believe, dark energy now accelerating it)
This expansion has two impacts. First, it increases the distance between objects and the bigger the distance between the two objects the faster the expansion - this expansion is a function of space-time, not a force on matter and photons etc. And space-time does not need to observe the constraint of the speed of light. Thus we suspect that the real universe is many times bigger than we can observe, because beyond a certain point the very distant universe would be expanding so fast that light emitted in a very distant part would never be able to reach us.
The second is that any photons emitted will get 'stretched' by this expansion and become red-shifted. Thus the earliest 'object' we can see is the cosmic microwave background radiation, which is the burst of light that decoupled when the universe cooled enough for neutral hydrogen to form - about 370,000 years after the big bang. At the time I believe it was a blackbody radiation at about 3000K. It is now a blackbody radiation of about 2.7K. In wavelength terms the photons have been stretched just over 1000 times in wavelength.
Thus the possibility that the James Webb telescope might see objects that formed in the very early universe - such as population III stars, because all the light emitted at that time will have been redshifted to infrared/microwave.
So TL;DR:
The expansion of the universe means that we are only
now getting light from certain parts of the universe, and it is these areas that we can see as they were at the earliest times.
Confusingly these areas are now much further away in real distance than the lifetime of the universe, but this can be accounted for by the expansion of the universe as well.
If you want a simple analogy. Think of a balloon that can be blown up indefinitely. Mark two spots on it. They are, say, galaxies A and B. The expansion of the universe is this balloon inflating constantly and getting bigger. As it does so the distance between A and B gets bigger. Now train an ant to walk between A and B at a constant speed - think of that as a photon being emitted from A towards B! As the expansion increases the distance the ant is still stuck at walking at the same speed, therefore will take longer to reach B.