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We present the first 3-dimensional simulations following the evolution ofsupernova shocks from their inception in the stellar core through thedevelopment of a supernova remnant into the Sedov phase. Our set of simulationsuse two different progenitors and two different conditions for the structure ofthe circumstellar environment. These calculations demonstrate the role thatsupernova instabilities (the instabilities that develop as the shock drivethrough the star) play in defining the structure and long-term development ofinstabilities in supernova remnants. We also present a first investigation ofthe mixing between stellar and interstellar matter as the supernova evolvesinto a young supernova remnant.

First Simulations of Core- Collapse Supernovae to Supernova Remnants with SNSPH