Fourier telescope is an imaging technique in which the Fourier spectrum of an object is built up by sweeping fringe patterns of varying spatial frequency and orientation over the object. The modulated scattered radiation that results is collected by a non-imaging detector. We have performed a laboratory demonstration of Fourier telescope in order to confirm the validity of the fundamental measurement concept and the image reconstruction method. We show experimentally obtained images and compare them to simulated images. On-going experiments will characterize the consequences of less-than-ideal measurement conditions. Our ultimate application is the imaging of geosynchronous satellites.