The measurement of the temperature of the cosmic microwave background
radiation (CMBR) with the Far InfraRed Absolute Spectrophotometer (FIR
AS) on the Cosmic Background Explorer (COBE) satellite gives a possibi
lity for determination of all mutually related parameters of the ultra
stable expansive nondecelerative Universe (ENU) with deviations smalle
r than 0.4%. The measurement of the large-scale anisotropy of the CMBR
with the Differential Microwave Radiometers (DMR) on the COBE satelli
te allows us to determine the mass density of gravitationally bound sy
stems of large-scale structures of the ENU.