From analysis of radial velocity measurements the binary nature of Ple
ione is discussed. A possible orbital period of about 35 yr was detect
ed. This value also coincides with the variations of the spectral prop
erties of the star (shell- non-shell phase). An elliptical orbit of hi
gh eccentricity (e > 0.75) is probable. The mass of the companion is p
robably not smaller than about 2.5 M..