We present the UBV observations of FG Sge performed on 55 nights in 19
96-1997 with three apertures: 27 '', 13 ''.5, and 10 ''. We measured t
he star together with part of the surrounding planetary nebula He 1-5
through the smaller apertures and the sum of three components-star + c
ompanion + nebula-through the large aperture. In 1996 the deepest mini
mum of all the five minima that had occurred since 1992, when the star
entered the R CrB phase, was observed.