We have measured the middle ultraviolet (MUV) electron impact induced fluorescence spectrum of SO2 from 200 to 430 nm in a crossed beam experiment. The spectrum is dominated by two features at the experimental resolution of 0.5 nm. These two features are referred to as MUV1 and MUV2. MUV1 is the SO(A3&Pgr;→X3&Sgr;-) band system extending from 240 to 265 nm produced by dissociating excitation. MUV2 is a blend of the SO2(A˜(1A2), B˜(1B1)→X˜(1A1)) and SO2+(C˜(2B2)→X˜(2A1 )) molecular band systems in the range 264-430 nm. In addition, the excitation function measurements of MUV2 indicate that low-energy electrons effectively prepare SO2 in one or more electronically excited triplet states that involve the SO2 (a˜(3B1)) state by direct excitation and/or cascading. A candidate triplet band system for this emission process is the E˜-a˜ electronic transition. This emission process is the largest contributor to the MUV2 emission cross section at low electron impact energy. The peak cross section for MUV1 occurs at 20 eV with a value of 25.0¿5.5¿10-19 cm2. The peak cross section for MUV2 arises at 9 eV with a value of 368¿81¿10-19 cm2. The laboratory measurements of the excitation functions of both MUV features were made from 0 to 1 keV. The emission cross sections are an important part of the total inelastic cross section of SO2 needed in modeling the Io atmosphere. The laboratory results give a plausible explanation of the Io auroral hot spots observed by Voyager 2. ¿ American Geophysical Union 1992