The amplitudes of peaks in the angular power spectrum of anisotropies in th
e microwave background radiation depend on the mass content of the universe
. The second peak should be prominent when cold dark matter is dominant but
is depressed when baryons dominate. Recent microwave background data are c
onsistent with a purely baryonic universe with Omega(m) = Omega(b) and Omeg
a(A) approximate to 1.