ALL STARS EXHIBIT INTENSITY FLUCTUATIONS OVER SEVERAL TIME SCALES FROM NANOSECONDS TO DAYS; THESE INTENSITY FLUCTUATIONS ECHO OFF PLANETARY BODIES IN THE STAR SYSTEM AND PROVIDE AN OPPORTUNITY TO DETECT AND IMAGE EXOPLANETS USING MODERN COMPUTATIONAL IMAGING TECHNIQUES. A MISSION UTILIZING DISTRIBUTED-APERTURE STELLAR ECHO DETECTORS COULD PROVIDE CONTINENT-LEVEL IMAGING OF EXOPLANETS MORE READILY THAN INTERFEROMETRIC TECHNIQUES AS HIGH TEMPORAL RESOLUTION DETECTION IS LESS TECHNICALLY CHALLENGING AND MORE COST EFFECTIVE THAN MULTI-KILOMETER-BASELINE FRINGE-TRACKING PARTICULARLY IN A PHOTON-STARVED REGIME. THE CONCEPT IS VIABLE FOR DETECTING EXOPLANETS AT MORE DIVERSE ORBITAL INCLINATIONS THAN IS POSSIBLE WITH TRANSIT OR RADIAL VELOCITY TECHNIQUES.