The CMB is composed of radiation with a black body distribution peaked at 
around 1000nm. The radiation is now in the microwave band at about 1 mm 
wavelength. The IR photons were spread by the expansion of spacetime by a 
factor of 1000, and the actual z factor for the CMB is z = 1100. With the 
exponential expansion of the universe this z will increase until the CMB is 
in the radio wave band > 1m wavelength, and then eventually expanded beyond 
the dimensions of any practical antenna. It will take about 10 billion 
years for that to happan.

LC

On Wednesday, December 27, 2017 at 2:17:49 PM UTC-6, agrays...@gmail.com 
wrote:
>
> Since galaxies were formed after the CMB came into existence about 380,000 
> years after the BB, and those far away will wink out as they cross the 
> cosmic horizon, why doesn't the CMB also wink out? I know the latter is 
> reddening as the cosmos expands, and is ubiquitous, but when the question 
> was posed to me last night at a meeting in Pasadena with former JPL 
> colleagues, I didn't have a good answer. TIA, AG
>

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