In March 2010 the Large Area Telescope on-board the Fermi Gamma-ray Space Telescope discovered for the first time >100 MeV gamma-ray emission from a nova within our galaxy, V407 Cyg. The high-energy spectrum and light curve was explained as a consequence of shock acceleration in the nova shell as it interacts with the local ambient medium. It was suspected that the necessary conditions for high-energy emission from novae would be rare. In June 2012 the LAT detected a new flaring source, Fermi J1750-3243, which is spatially coincident and contemporaneous with a new nova, Nova Sco 2012. We report on the exciting discovery of this new, 'gamma-ray' nova and present a detailed analysis of its high-energy properties.