The aim of the present letter is to critically review the stability of
the Bartnik-McKinnon solutions of the Einstein-Yang-Mills theory. The
stability question was already studied by several authors, but there
seems to be some confusion about the nature and the number of unstable
modes. We suggest to distinguish two different kind of instabilities,
which we call ''gravitational'', respectively ''sphaleron'' instabili
ties. We claim that the nth Bartnik-McKinnon solution has exactly 2n u
nstable modes, n of either type.