  We present high resolution VLT UVES observations of the active K dwarf GJ
117. 6^Li enhancement has been shown for energetic solar events, one
chromospherically active binary, and several dwarf halo stars. Our analysis
reveals the detection of 6^Li on this source with 6^Li/7^Li = 0.030+/-0.010. We
found no significant contribution from other lines, including Ti I, in the Li
profile of GJ 117 and a template star of similar spectral type and metallicity.
We discuss the possibility for 6^Li production by spallation and find it to be
consistent with the activity levels of the object.
