In this talk, I explore the anisotropies of the Cosmic Microwave Background in the presence of massive, decaying neutrinos. The effects on the anisotropies are very different for different neutrino masses and lifetimes. For long lifetime, low mass neutrinos, and for short lifetime, low mass neutrinos, the anisotropies differ only slightly from the massless, non-decaying case. I examine the distinguishability of these models in light of future satellite-based experiments, MAP and Planck. Another case involves a neutrino species of mass greater than 10 eV with lifetime between 10^{13} sec and 10^{17}. Here the anisotropies at large angles are predicted to be comparable to those on degree scales, due to the ISW effect. Present data exclude such a possibility and hence this region of parameter space.