Gliese 268 [SEP] constellation
Gliese 268
Gliese 268 (QY Aurigae) is a RS Canum Venaticorum variable (RS CVn) star in the Auriga constellation. RS CVn variables are binary star systems with a strong magnetic field influenced by each star's rotation, which is accelerated by the tidal effects of the other star in the system. Gliese 268 in particular is composed of a binary system of two M-type dwarfs, or red dwarfs, and is one of the one hundred closest star systems to the Earth. The primary component of the system
Gliese 105
Gliese 105 (also known as 268 G. Ceti) is a multiple star system in the constellation of Cetus. It is located relatively near the Sun at a distance of 23 light-years (7 parsecs). Despite this, even the brightest component is barely visible with the unaided eye "(see Bortle scale)". No planets have yet been detected around any of the stars in this system.
This is a triple system with three stars that are all less massive than the Sun. The