Radial velocity variations of the K supergiant Xi Cygnl are Investlgated on the basis of publlshed as well as new values from spectrograms In the visual and near infrared region obtalned In the period of 1977-1984 at Ondřejov, Shemakha, and Crlmea observatories. A circular orbit (P = 113.3873 days, Tmax = 2430214.33 HJD, K1 = 3,47 km/s, Vo = -20.0 km/s), still preliminary. confirms the period derlved by Parsons (1983). More accurate data are needed and the problem of the long period (Reimers 1981)
should be investigated.