Apparently I drifted off at the end of my last post. I meant to say something like
The balloon model is a very good analogy to cosmological expansion. I think understanding it would answer a lot of your questions.
[QUOTE=Frylock]
When we detect the CMB, does the CMB look to us as though it is 14 billion years old or 46 billion years old? In other words, here are the two scenarios I am envisioning:
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When we do whatever it is we do to measure the distance of the CMB, we get 14 billion–but we know how space has expanded over the past 14 billion years so we know it’s actually 46 billion light years away.
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When we do whatever it is we do to measure the distance of the CMB, we get 46 billion.
Is one of these correct, or neither somehow?
[/QUOTE]
At this point it probably won’t surprise you too much that the answer is “Neither, really.” At any rate, the CMB is just made up of photons; they have no measurable age (and in their reference frame, they do not age at all). They have a wavelength, a direction, and a polarization, and that’s it. The raw measurements of the CMB are measurements of a blackbody spectrum, which is basically measuring the intensity of the radiation as a function of frequency (like here). To get any measurement of distance or age out of this, we need more information.
For the CMB, one piece of extra information is the initial temperature of the radiation. This radiation is believed to come from a proton-electron plasma just before recombination, and theory gives estimates for how hot that plasma must have been. The ratio of this temperature to the measured CMB temperature then tells us how much the radiation has been redshifted on its journey (specifically, this is the expansion factor 1+z for the CMB).
(Similar but different tricks are used to get redshifts to other sources. In some cases the source has well-known emission lines which can be identified at a different wavelength than they actually emit at. In some cases, clouds somewhere between us and the source can form absorption lines, which at least gives a lower bound on how far away the source is.)
This is still not a distance or an age. To go further than this, a model of the evolution of the universe is needed. In the case of the CMB, some of the extra information is actually in the anisotropy of the radiation, which gives information about how large the surface was at last scattering. To convert this result to a comoving distance as Stranger has done, you need to further know something about how the universe has evolved between then and now.
If all of this seems a terribly oblique and roundabout way of measuring simple quantities… welcome to cosmology, where the definitions of “distance” take a chapter or so. The problem of measuring distances in cosmology (the “distance ladder”) is very old and not at all straightforward.