40 Eridani A is a
main-sequence dwarf of
spectral type K0.5, 40 Eridani B is a 9th magnitude
white dwarf of spectral type DA4, and 40 Eridani C is an 11th magnitude
red dwarf flare star of spectral type M4.5e. When component B was a main-sequence star, it is thought to have been the most massive member of the system at , but ejected much of its mass before it became a white dwarf. wider than the Sun does on Earth. An observer on a planet in the system would see the B–C pair as unusually bright white and reddish-orange stars in the night sky –
magnitudes −8 and −6, slightly brighter than the appearance of
Venus seen from Earth as the
evening star. It is unlikely that habitable planets exist around because they would have been sterilized by its evolution into a white dwarf. As for , it is prone to flares, which cause large momentary increases in the emission of
X-rays as well as visible light. This would be lethal to
Earth-type life on planets near the flare star. ==Search for planets==