Wow MA, I don't know where to begin... :shock:
Lets start with your statement -
"the edge of the Observable Universe is that distance from us at which everything is moving away at c relative to us".
Firstly, do you mean "is moving away at c" right now, or was moving away at c when the light we see was emitted? Do you mean the Hubble distance "then", or the Hubble distance "now"?
The Hubble distance was 5.7 billion light-years when the light we see was emitted from galaxies that were receding at
c and that light has a redshift of a little over z=1.4, which means those regions have receded to around 14 billion light-years away by now, due to the expansion of the universe. But that light was
only emitted a little over 9 billion years ago.
We have seen light that has been travelling for
much longer than that, and thus has covered a greater distance. Photons from more distant galaxies were just passing those galaxies at the edge of our Hubble sphere 9 billion years ago!
We have seen galaxies at redshift z=7, whose light has been travelling for nearly 13 billion years. Their light was travelling for around 4 billion years before it overtook those galaxies at z=1.4 and crossed into our Hubble sphere. From our point of view, the light from those z=7 galaxies was receding from us for 4 billion years, as the space it was travelling through was receding from here superluminally. As the rate of expansion decelerated, that light eventually found itself in regions of space that were receding from here at less than the speed of light, as it passed into our Hubble sphere, 9 billion years ago.
We have seen the light from galaxies that were receding at multiples of c when that light was emitted, so how can the distance where an object did, or does, recede at c, be considered the edge of our observable universe?
It's late now, I'll leave the part about the infinite void till tomorrow.