In this paper we rule out the possibility of asymptotically selfsimilar singularities for both of the 3D Euler and the 3D Navier-Stokes equations. The notion means that the local in time classical solutions of the equations develop self-similar profiles as t goes to the possible time of singularity T . For the Euler equations we consider the case where the vorticity converges to the corresponding self-similar voriticity profile in the sense of the critical Besov space norm,Ḃ 0 1,∞ (R 3 ). For the Navier-Stokes equations the convergence of the velocity to the self-similar singularity is in L q (B(z, r)) for some q ∈ [2, ∞), where the ball of radius r is shrinking toward a possible singularity point z at the order of √ T − t as t approaches to T . In the L q (R 3 ) convergence case with q ∈ [3, ∞) we present a simple alternative proof of the similar result in [16]. *