ealia said:
That is very interesting marcus. If you could please, I would very much like to hear how that occurs - I have not heard of it before. Thanks. :)
Maybe you already know this: cosmo is a math science. Everything we say is about a model. The model is very simple and is built into calculators.
With purely verbal explanation there is little gain in understanding. To learn you need hands-on experience with the calculator (or the Friedman equation that it is based on.)
I don't know you. You may be smart on a math level (as well as on verbal level). You may have already tried Siobhan Morgan's calculator, that I was urging in post #11 and again in post #15.
If not, my verbal explanation might not help. But if you listen and ALSO play with the calculator it might work.
The Friedman eqn governs H(t) and you can see that H must always decrease.
But if you played with the calculator you would have ALREADY SEEN that H decreases over time. As you plug in higher and higher redshift the age of the universe goes down and down and the calculator TELLS YOU what H is at each age of the U. H goes up as you go back in time.
Take a pencil and make a table showing how as the age increases---1 billion 2 billion 3 billion...---the Hubble rate is decreasing. Quite sharply at first!
Now there is some algebra which a 14 year old can do.
The key equation is v = HD. What distance corresponds to v = c?
That is
the distance that is growing at exactly rate c. Larger distances grow faster. Smaller ones no so fast.
The 14 year old child tells you the critical distance is c/H.
If the photon aimed at us can ever get to within distance c/H of is, it will make it!
But I told you H was decreasing. You can and should check it with the calculator.
Therefore the critical distance is INCREASING.
All the photon has to do is hang in there and stay roughly the same distance from us (or even be swept back a iittle), for long enough, and the critical distance will REACH OUT TO IT. And then it is safe. It will be within the sphere of distances that are NOT increasing faster than c. And it will begin to make real progress and reduce the distance it needs to go and actually gain ground.
So say the distance to the galaxy is increasing at 1.1 c and it emits a photon in our direction. The distance to the photon will then be only be growing at 0.1 c
It has a fighting chance. It keeps on struggling towards us and only gets swept back slowly, at 0.1 c.
Now the critical distance c/H is reaching out very fast because (as you can see by experimenting with the calculator) the denominator H is decreasing rapidly. After a while if the photon keeps trying, it will be within the magic circle. So even though it has to fight the expanson of distances, the photon will eventually get to us.
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The whole thing depends on H decreasing and now it is decreasing much more slowly than it did earlier when expansion was only a few billion years old. So this opportunity is shrinking. Eventually the trick will not work or will do so only in a very marginal way. Too bad. But that is still far in the future.
Our sky is still full of galaxies that emitted light to us when they were receding >c and the light is still getting to us.
The time will come when there are not so many galaxies visible in the sky. But it is far in the future so not to worry.
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You should be able to calculate the critical distance c/H.
c is 300,000 km per second
H is 71 km per second per megaparsec (a unit of distance)
So c/H would be some number of megaparsecs that you can calculate.
I invite you to find that number of megaparsecs. Google will convert it to other units like meters or miles or lightyears, if you want.
Whatever that distance is, distances bigger than it are increasing >c
and distances smaller than it are increasing slower than c.
Very important distance. It has a special name: Hubble radius.
Maybe you knew all that. If you didn't, and have never calculated the Hubble radius, why not try?
Confucius is alleged to have said: "Tell me and I will forget. Show me and I might remember. Involve me and I will understand." John Dewey the American philosopher said "learn by doing" or words to that effect

I was just reading the Wikipedia on "experiential learning". Did you ever read anything about that?