  We present infrared observations of the young, oxygen-rich supernova remnant
1E 0102.2-7219 (E0102) in the Small Magellanic Cloud, obtained with the Spitzer
Space Telescope. The remnant is detected at 24 um but not at 8 or 70 um and has
a filled morphology with two prominent filaments. We find evidence for the
existence of up to 8x10^-4 Msolar of hot dust (T~120 K) associated with the
remnant. Most of the hot dust is located in the central region of E0102 which
appears significantly enhanced in infrared and radio continuum emission
relative to the X--ray emission. Even if all of the hot dust was formed in the
explosion of E0102, the estimated mass of dust is at least 100 times lower that
what is predicted by some recent theoretical models.
