  We develop some properties of the non-BPS attractive STU black hole. Our
principle result is the construction of exact solutions for the moduli, the
metric and the vectors in terms of appropriate harmonic functions. In addition,
we find a spherically-symmetric attractor carrying $p^0$ ($D6$ brane) and $q_a$
($D2$ brane) charges by solving the non-BPS attractor equation (which we
present in a particularly compact form) and by minimizing an effective black
hole potential. Finally, we make an argument for the existence of multi-center
attractors and conjecture that if such solutions exist they may provide a
resolution to the existence of apparently unstable non-BPS ``attractors.''
