  In March 2010 the Large Area Telescope (LAT) 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, that 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.
