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The cosmic microwave background radiation is the furthest and oldest visible light in the universe. But the universe has expanded considerably since that light was emitted. At the time that that light was emitted, how big was the “thing” that emitted that light? Was it bigger than, say, the Milky Way?

And, how should I conceptualize the object? I imagine it as a growing sphere of light, but that presumed that it was expanding into something… But since (perhaps?) this thing was space itself, then maybe it doesn’t have a surface. Could it nevertheless be described as a finite volume, just, perhaps one without a boundary? And if so, how on earth do I visualize that?

  • The diagram here may help: https://physics.stackexchange.com/a/659681/123208 – PM 2Ring Nov 25 '23 at 06:58
  • The CMB filled the entire (observable and, in theory, non-observable) universe then, and it fills the entire universe now. There was and is no surface. – Ghoster Nov 25 '23 at 07:15
  • Possible duplicate: https://physics.stackexchange.com/a/621281/123208 – PM 2Ring Nov 25 '23 at 07:25
  • @Ghoster The CMB radiation that we're receiving right now comes from a spherical surface, roughly speaking. It's not exactly a spherical surface because the transition from opaque to transparent wasn't instantaneous, it took several thousand years. – PM 2Ring Nov 25 '23 at 07:31
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    @PM2Ring Agreed… the surface of last scattering. I meant all the CMB fills the universe. – Ghoster Nov 25 '23 at 07:32

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