  The expansion of the universe may be observed in ``realtime'' by measuring
changes in the patterns of the anisotropy in the CMB. As the universe ages, the
surface of decoupling--or the CMB photosphere--moves away from us and samples a
different gravitational landscape. The response of the CMB to this new
landscape results in a different pattern than we observe today. The largest
change occurs at l~900. We show that with an array of detectors that we may
envision having in a couple of decades, one can in principle measure the change
in the anisotropy with two high precision measurements separated by a century.
