Chi1 Orionis
Chi Orionis (χ Ori, χ Orionis) is a star about 28 light years away. It is in the constellation Orion, where it can be seen in the tip of the Hunter's upraised club. χ Ori is a G0V star. It has a faint companion with a mass estimated at about 15% of the mass of the Sun, and an orbital period of 14.1 years. The companion orbits an average distance of 6.1 AU from the primary, but has a fairly high orbital eccentricity, ranging from 3.3 AU out to 8.9 AU from the primary. Because of this  red dwarf companion, the likelihood of habitable planets in this system is low. It is thought that the companion is a red dwarf still contracting towards the main sequence. A necessary condition for the existence of a planet in this system are stable zones where the object can remain in orbit for long intervals. For hypothetical planets in a circular orbit around the individual members of this star system, this maximum orbital radius is computed to be 1.01 AU for the primary and 0.41 AU for the secondary. (Note that the orbit of the Earth is 1 AU from the  Sun.) A planet orbiting outside of both stars would need to be at least 18.4 AU distant. χ Ori is a candidate stream star member of the Ursa Major Moving Group, although there is some evidence to the contrary.