For those whose tastes run to explosions, classical novae are a goldmine of physical processes whose study illuminates a broad range of comic objects: planetary nebulae and luminous blue variables in fast forward, supernovae in slow motion, and lots in between. I'll review some of the results of the last seven years of panchromatic observations and simulations that are the basis of the Nova Legacy Project, a coordinated benchmark study of every known subtype of nova from cm through MeV.