Spectral energy distribution of a star with ﹩T=5800﹩ K surrounded by a dusty debris disk with ﹩T=80﹩ K. This system is put at the Galactic center (distance ﹩D=8﹩ kpc). The reflected (dashed curves) and reemitted (dotted curves) lights from the disk are calculated for three values of the disk‐to‐star luminosity ratio: ﹩\tau =10^{-2}﹩, 10⁻³, and 10⁻⁴.