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Although designed to study solar flares, the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI), a NASA satellite, has proven to be sensitive to γ-ray lines generated by recently created radionuclei in the inner Galaxy. I present the current state of this investigation, including flux and line shape measurements of the 1809 keV line from 26 Al and a preliminary detection of the lines of 60 Fe.