The primary star Gliese 569A is a flare star. The star was given its variable star designation, CE Boötis, in 1975. The nature of the brown dwarf binary Gliese 569B is highly uncertain, and it was even suspected Gliese 569Ba itself may be either a low-mass star or a binary object. But with a mass about 8-9% that of the Sun means it may possibly be a binary of two extremely low massultra-cool dwarf stars that are extremely dim, dim enough to look like a brown dwarf. Both browndwarfs are weakly variable, likely due to starspot activity.