The next eclipsing variable star from the constellation of the Kids, with a magnitude change from 3.9mag to 4.2mag in a period of 2.66 years - 972.18 days, with the second longest known period. The brightness decrease from maximum to minimum, or the increase from minimum to maximum, lasts only a few days, and the star remains at minimum for 38 days. The main component is red, the secondary component is blue. Sometimes, faint blue stars come to us through the outer layers of a red giant, creating interesting spectroscopic phenomena.