darkmatter4brains wrote:ramparts wrote:SpeedFreek wrote:Cosmological time (and the age of the universe) is an approximation, based on a theoretical series of clocks in free-fall across time, under the least gravitational influence in their own epoch, co-moving with the expansion of the universe.
Beautifully put!
ah yes, and this reminded me how this is all related to the CMB!
When measured from Earth, the CMB (Cosmic Microwave Background) Radiation does look a tad warmer in one direction than it does in the other. This is because Earth is not perfectly comoving with the expansion of the Universe. It's in orbit around the Sun; The Sun "orbits" around in the Milky Way galaxy on one of the rings. And, the Milky way even has some overall motion towards the Hydra cluster.
The CMB exhibits the highest degree of homogeneity (and isotropy, really) in the frame that is comoving with the expansion of the Universe. Any measured change in this homogeneity would indicate that the frame from which you have measured it in, has some motion away from the expansion of the Universe.
The fact that the CMB is homogenous across the entire Universe, lets us be able to confidently define an age for the Universe that EVERYBODY, ANYWHERE can agree upon. Almost sounds "absolute" doesn't it!!
Actually, it almost sounds like the ether. But, not quite, thank goodness
Indeed - due to large-scale homogeneity and isotropy, we can talk about a CMB rest frame (in which the dipole you mentioned disappears). This is the closest we have to an "absolute" frame of reference in the universe - technically it's not actually privileged above any other reference frame, but we can treat it as such since it is unique in that the whole universe looks the same from it. </science>



