The article offers information on the eclipsing binary system Epsilon Aurigae which has intrigued astronomers for 150 years. The bright 3rd magnitude star of the Epsilon Aurigae is close to Capella and the primary component is the supergiant F star with 1-astronomical unit (AU) radius. Astronomers are fascinated by the 2-year length of the Aurigae eclipse and the brightness of the system at mid eclipse.