THE INFRARED TEMPORAL EVOLUTION OF FG SAGITTAE

We present near- and mid-infrared photometry of the post-AGB star FG S ge obtained at two distinct epochs separated by a period of 10 years. Observations of FG Sge taken in 1983 suggest that the 1 to 12 mum ener gy distribution was produced at that time by a stellar photosphere, wi th a blackbody temperature of almost-equal-to 5600 K. In late August o f 1992, FG Sge exhibited a marked decline (almost-equal-to 3 mag in V) in its visible light curve. At the same time the 1 to 18.0 mum infrar ed energy distribution has evolved to become a almost-equal-to 1000 K blackbody. We propose that this light decline partially is due to the ejection and condensation of a dust shell. We estimate the amount of d ust condensed during this episode to be almost-equal-to 3.3 x 10(-9) M ., with a covering factor (total visual depth) of almost-equal-to 0.3.