This paper sets out to develop a vector field theory of time‐dependent backscatter from a large target and shows how the cross‐polarization of the return signal follows as a natural consequence of certain spatial asymmetry of the target with respect to the illuminating source. It presents an analysis of radar backscattered power from a distant, slightly rough sphere for both pulsed and sinusoidally steady‐state sources. At first, an integral expression for the received power is developed for an arbitrarily rough sphere. Then the height deviation from the mean sphere is specialized to have a bivariate Gaussian distribution and a Gaussian correlation function. The average direct‐ and cross‐polarized received powers are derived for both the pulsed and the steady‐state cases. Numerical results are computed for the case of a very slightly rough sphere for which σ/δ is of the otder of 10‒4 and presented in contrast with experimental data from a target with a much larger scale roughness, namely the moon. (In this paper σ represents the standard deviation of heights and δ is the correlation distance.)