The mass of the universe has often been cited to be approximately 1053 kg, [1-3] a finite number. Current values are derived from either critical density estimations, the average number of stars including interstellar and intergalactic matter, or Hoyle based steady-state estimates, and all imply a finite universe.If the universe is somehow (as thought) accelerating, then a force is somehow (as Max Planck insisted) being applied, yet what force, and how? We know that as a whole, the universe seeks equilibrium. Specific, temporary, or local trajectories and/or accelerations may achieve partial equilibriums, and lead to further “adjustments” in differing magnitudes. Where, again the seeking of equilibrium continues. In the end, the universe as a whole can be seen as being in a multiple state (or in multiple phases) of continuously seeking both partial and complete equilibriums. This conclusion is remarkable; it implies that some partial equilibrium is already achieved, for it “continuously” seeks equilibriums, yet it also implies that the universe is actively seeking some quotient of further equilibrium. It is this partial, already achieved, yet integral equilibrium which this paper describes.