The latest results on the spectrum and anisotropy of the microwave bac
kground from the COsmic Background Explorer (COBE) are discussed. The
RMS deviation of the spectrum from st 2.728 +/- 0.004 K [95% CL] Planc
k function is less than 50 parts pm million of the peak intensity. Ene
rgy added to the CMBR by hot electrons (y and mu distortions) is less
than 60 parts per million [95% CL] of the total CMBR energy for all ti
mes later than 1 year after the Big Bang. The anisotropy of the CMBR i
s consistent with a power law power spectrum of primordial density per
turbations with P(k) proportional to k(n), and the spectral index n =
1.2 +/- 0.3 (1 sigma), consistent with the n approximate to 1 predicte
d by inflation. The amplitude of power spectrum gives an expected RMS
quadrupole of (Q(RMS)(2))(0.5) = 18 mu K if n is forced to be 1.