DISCOVERY OF AN EXTENDED NEBULA AROUND AFGL-2343 (HD-179821) AT 10 MICRONS

We present images at 8.5, 10.5, and 12.5 mu m which reveal that AFGL 2 343 (HD 179821) is surrounded by a dusty nebula 4 ''-5 '' in diameter at 10.5 and 12.5 mu m. This G5 Ia supergiant has long been suspected o f having a detached dusty envelope because of its optical brightness a nd large IR excess. The nebula is ringlike and slightly elongated, wit h bright patches or clumps to the northeast. An 8.5 mu m image is domi nated by the photosphere of the central star, which also appears to a lesser extent in the 10.5 and 12.5 mu m images. A full radiative trans fer model of the nebula correctly predicts the observed inner (1 ''.1) and outer (1 ''.9) radii of the shell and the spectral energy distrib ution of the shell. With the aid of this model, we find that AFGL 2343 is almost certainly an extremely massive star at a distance of about 6 kpc, which has recently undergone an enormous mass-loss event, durin g which M = 10(-2) M. yr(-1), while the current mass-loss rate is less than 2 x 10(-6) M. yr(-1).