  The new spatial condensation cosmological theory, based on the new universal
constant of expansion, kappa = G Rho t^2 = 3/(32 Pi), is used to predict
measurements of the supernova Ia data with no acceleration of the expansion
rate of the universe. That goal was accomplished with the key assumption that
radiation travels on great circles on the surface of the supporting 4-D ball
towards the detector at the compounded velocity of Vc = Hr - c. The radiation
has traveled great distances from emission to measurement in the expanding
universe and is exactly suited to test the global predictions of a cosmological
theory. Problems of the current big bang theory are discussed. It will be shown
that a new method of analyzing the data does indeed show the simplicity and
consistency of the new theory in contrast to the old Friedmann big bang model.
