  We show that a contribution to the total curvature perturbation may be due to
the presence of flat directions in supersymmetric models. It is generated at
the first os- cillation of the flat direction condensate when the latter
relaxes to the minimum of its potential after the end of inflation. We also
point out that, if the contribution to the total curvature perturbation from
supersymmetric flat direction is the dominant one, then a significant level of
non-Gaussianity in the cosmological perturbation is also naturally expected.
