The current outburst of Delta Sco, and the circumstances of its discovery, remind me very much of a somewhat similar experience I had many years ago. In 1978 I stumbled upon the star HD 96446 in Carina. Its published spectral type was B2 IIIp (or B2 V He, or B3 Vp). Its accepted magnitude was V=6.68. But on observing it on 1978 April 10, there it was- a full half-magnitude brighter than that, at 6.2. This star is in a rich part of the Carina milky way, with numerous other V magnitudes around it for comparison. I started observing this star regularly, and its remained bright for at least 30-40 days, but then commenced a slow, erratic fade. About 90 days after my first observation it had faded back to its normal level of 6.7. That was in the 1978 observing observing. In the 1979 observing season I continued to follow it, and I think I observed a smaller brightening, by no more than 0.3 mag, which may have lasted for 80-90 days. Strangely to say, HD 96446 eventually received a variable star name - V430 Car, but _not_ because of my observations. It was found to be a small amplitude (0.03V) variable of the Beta Cephei type by Matthews and Bohlender (1988, IBVS 3226). At the time of my discovery, I did contact a couple of observatories, and apparently someone did try to carry out p.e. observations, and possibly also spectral observations, which would have been very useful in confirming the outburst. I have never seen the results of such observations, and the only continuous record I have are my own visual estimates. A complete report on the outburst of V430 Car is given in PUBLICATIONS of the Variable Star Section of the Royal Astronomical Society of New Zealand, No. 18 (1992), pp 17- 21. It includes a light curve. Cheers, Mati Morel Astrographics c/o M. Morel, 6 Blakewell Rd, Thornton NSW 2322 AUSTRALIA *Specialized Charts** Variable Star Studies** Stellar Data** 151o38'33" E, 32o46'47"S. morel@ozemail.com.au