  A collection of requirements to the General Relativity that follow from the
WMAP observations of the Cosmic Microwave Background radiation anisotropy as an
inertial frame are discussed. These obligations include the separation of both
the CMB frame from the diffeomorphisms and the diffeo-invariant cosmic
evolution from the local scalar metric component in the manner compatible with
the canonical Hamiltonian approach to the Einstein--Hilbert theory with the
energy constraints. The solution of these constraints in classical and quantum
theories and a fit of units of measurements are discussed in the light of the
last Supernovae data.
