Hi, all: Gathering delta Scorpii's data, I realized that the only other time when the star was measured brighter than normal (V= 2.21 instead of 2.32) was back in 1958.(Hogg A.R.). Taking the orbital period from Fabregat, Reig and Tarasov (2000) P= 10.583 and the ephemeris from Hartkopf et al., (1996) To = 1979.41 , we find that another periastron passage had taken place in 1958.24. It is very interesting to find this, because it's a very good indicator of the relation between the binary nature of the system and the observed events. Cheers, Sebastian Otero, LIADA, Buenos Aires, Argentina.