We compute the skewness of the matter distribution arising from nonlinear e
volution and from non-Gaussian initial perturbations. We apply our result t
o a very generic class of models with non-Gaussian initial conditions and w
e estimate analytically the ratio between the skewness due to nonlinear clu
stering and the part due to the intrinsic non-Gaussianity of the models. We
finally extend our estimates to higher moments.