Description
The Sudbury Neutrino Observatory (SNO) is a heavy water Cerenkov detector located deep underground in the Creighton mine in Canada. Its recent dramatic results have solved the "solar neutrino problem" with the demonstration of neutrino oscillations and neutrino mass. SNO is now in the third and final phase of operations. I will review the current status and our results to date. I will also present the status of the new SNOLab facility, dedicated to an ongoing astroparticle physics program including low energy solar neutrinos, neutrinoless double beta decay, and searches for dark matter