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The question of the nature of the progenitor of Type Ia supernovae (SNe Ia)is important both for our detailed understanding of stellar evolution and fortheir use as cosmological probes of the dark energy. Much of the basic featuresof SNe Ia can be understood directly from the nuclear physics, a fact whichGerry would have appreciated. We present an overview of the currentobservational and theoretical situation and show that it not incompatible withmost SNe Ia being the results of thermonuclear explosions near theChandrasekhar mass.

SNe Ia: Can Chandrasekhar Mass Explosions Reproduce the Observed Zoo?