Epsilon Reticuli

[10] The brighter star should be easily visible without optical aid under dark skies in the southern hemisphere.

The primary component, Epsilon Reticuli A, is a subgiant star with a stellar classification of K2III–IV, indicating that the fusing of hydrogen in its core is coming to an end and it is in the process of expanding to a red giant.

[11][12] It was noted that its color indices are incompatible with a main sequence object, but are consistent with a white dwarf.

[12] This was confirmed in 2007 by spectroscopic observations, that showed the absorption spectrum typical of a hydrogen-rich white dwarf (spectral type DA).

[14] With a minimum mass of 1.17 that of Jupiter, the planet moves around Epsilon Reticuli with an average separation of 1.16 AU.

The inner Solar System superimposed behind the orbits of the planet Epsilon Reticuli b (and several others)