EPSILON ARIETIS

'Epsilon Arietis' (ε Ari / ε Arietis) is a triple star system in the constellation Aries. It is approximately 293 light years from Earth.
The two brightest components, 'ε Arietis A' and 'B', are both white A-type main sequence dwarfs with apparent magnitudes of 5.2 and 5.5 respectively. They are separated by 1.5 arcseconds on the sky. The third component, 'ε Arietis C', is 146 arcseconds from A and has an apparent magnitude of 12.7. The combined apparent magnitude of the system is +4.63.