Epsilon Reticuli

Stellar classification



  • X 44
  • Y -40
  • Z 0
→ Sol: 59

Object type

  • High proper-motion Star
  • Star
  • Double or multiple star
  • Infra-Red source
  • UV-emission source
simbad:* eps Ret


Epsilon Reticuli (Epsilon Ret, ε Reticuli, ε Ret) is a double star approximately 59 light-years away in the constellation of Reticulum. The primary component is an orange subgiant, while the secondary is a white dwarf. The two stars share a common motion through space and hence most likely form a binary star system. The brighter star should be easily visible without optical aid under dark skies in the southern hemisphere. In 2000, an extrasolar planet was confirmed to be orbiting the primary star in the system.

This article uses material from the Wikipedia article "Epsilon Reticuli", which is released under the Creative Commons Attribution-Share-Alike License 3.0.