COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS _ NUMBER 402 Konkoly Observatory Budapest 1969 November 11 V-OBSERVATIONS AND LIGHT ELEMENTS OF OMEGA Cen V78 V photographic observations (Kodak 103aD + Shott filter) of the eclipsing binary V78 in Omega Centauri were obtained at the Bosque Alegre Observatory with the 1.54 m reflecting telescope. Magnitudes were measured with a Zeiss iris-diaphragm photometer. They are in Woolley's system (Woolley, 1963) which is based on Eggen's photoelectric sequence (Eggen, 1963), [FIGURE 1] Figure 1. V-Observations of V78 in Omega Cen Three times of minimum were obtained. They were derived from comparisons of individual observations at primary minimum with a mean light curve. Older Bpg minima (Sistero, 1968) and the three recently obtained are as follows: Minima E (O-C) JD hel. 2429470.3099+-0.0067 m.e. -6388 +0,009 2427895.4195+-0.0036 -5166 -0,001 2427943.3090+-0.0015 -5125 -0,002 2427970.1714+-0.0037 -5102 -0.007 2440055.6397+-0.0032 +5244 -0.001 2440299.7790+-0.0099 +5453 -0,001 2440395.5855+-0.0088 +6535 -0.001 2440409.5882+-0.0077 +5547 +0.004 A least squares solution gives the light elements: Min = JD hel. 2433929.9724 + 1d16812901. E +-.00 +-000000 p.e. The V-light curve (Fig. 1) is similar to the B already obtained; though, the V observations are not sufficient, especially at maximum, as to derive orbital elements. As Omega Cen is kept under observation we hope to cover the entire cycle by the next observing season. 1969 November 3 R.F. SISTERO* C.R. FOURCADE* J.R. LABORDE Cordoba Observatory and I.M.A.F. * Laprida 854, Cordoba Argentina Reference: Eggen, O., 1963, unpublished, results given in Woolley, 1963. Sistero, R.F., 1968, I.B.V.S. Comm.27 I.A.U. No 316. [IBVS 316] Woolley, R.v.d,R., 1963, Roy.Obs.Ann., No 2,