COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 503 Konkoly Observatory Budapest 1971 January 4 A LIKELY 15.5 YEAR APSIDAL MOTION PERIOD IN HS Her The purpose of this note is to draw attention to HS Her: an eclipsing binary which seems to have an apsidal motion period of only 15.5 years. A complete discussion will be published later. Times of primary (and secondary) minimum observed in the next very few years could confirm this value. A 15.5 year apsidal motion period would be the shortest known, the shortest until now being the 25-year period of GL Carinae. HS Her is ideal for observing. It is bright (V=8.6m at maximum); the orbital period is short and convenient (P = 1.64d); the eclipses are brief (D = 5h); and both minima are reasonably deep (DeltaV pri = 0.50m and DeltaV sec = 0.15m), All of the data available at this time can be satisfied only by the following ephemeris for primary minimum, with the sine term; attributed to apsidal motion: Hel.JD = 2 437 854.194+1.6374333d E+0.017d sin (E/3450-360d) These data include spectroscopic orbital elements (Cesco and Sahade 1944) and times of minimum, both published (Martynov 1940, 1951; Hall 1967) and unpublished (Hall and Hubbard 1970; Atkins and Devinney 1970; and Martynov 1970). The above ephemeris predicts there should be no displacement of secondary minimum with respect to primary in the simmer of 1971, when HS Her next becomes observable. But after that, for the next 7 or 8 years, secondary minimum should occur later than 0.50p. DOUGLAS S. HALL Dyer Observatory Vanderbilt University Nashville, Tennessee 37203 U.S.A. References Atkins, H. and Devinney, E.J., Jr. 1970. private communication. Cesco, C. and Sahade, J. 1945, Ap.J. 101, 114. [BIBCODE 1945ApJ...101..114C ] Hall, D.S. 1967, P.A.S.P. 79, 444. [BIBCODE 1967PASP...79..630H ] Hall, D.S. and Hubbard, G.S. 1970. in preparation. Martynov, D.Ja. 1940, Bull Astr.Obs. V.P. Engel'gardta, No. 18, 38, Martynov, D.Ja. 1951, Izv.Astr.Obs.V.P. Engel'gardta, No. 26, 47. Martynov, D.Ja. 1970, private communication. [From IBVS 523] Correction to IBVS No 503 (HS Her): The last term in the equation should read: +0.017d sin (360d E/3450)