Black hole quasinormal modes are governed by a non-normal evolution operator with respect to a natural choice of inner product, and thus do not form a complete and orthogonal basis. In this talk, I will exemplify this mechanism by discussing a transient form of superradiance, drawing similarities to the transition to turbulence in Navier-Stokes this talk, I will exemplify this mechanism by discussing a transient form of superradiance, drawing similarities to the transition to turbulence in Navier-Stokes shear flows.