The results of UBV observations of FG Sge, performed in 1994-1995 thro
ugh three apertures: 27'', 13''.5, and 10'', are presented. With the s
maller apertures, the star was measured together with part of the plan
etary nebula He 1-5 surrounding FG Sge; with the large aperture, the s
um of the fluxes from three components was measured: star + companion
+ nebula In 1994, two more deep light minima were observed in the star
, in addition to the minimum of 1992.