The Epsilon Indi System (IMAGE) Carnegie Institution for Science Caption Artist's conception of the Epsilon Indi system. The two brown dwarfs orbit their common center of mass, which in turn orbits the much more distant primary component, a Sun-like star. By mapping the orbital motion of the brown dwarfs, the team was able to determine their masses. Much like our Solar System's giant planets, brown dwarfs are thought to have cloud belts that encircle the entire object and give it a striped appearance. Credit Illustration is by Roberto Molar Candanosa and Sergio Dieterich, courtesy of the Carnegie Institution for Science. Usage Restrictions With credit. License Licensed content Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.