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A supernova remnant is the expanding stellar debris and shocked surrounding gas left by a supernova. The debris drives an outward shock wave into the ambient interstellar medium; a reverse shock wave heats the ejecta as the expansion is decelerated. Hot plasma emits X-rays, while accelerated electrons produce synchrotron radiation in the magnetic field. Comparing successive images measures expansion, and X-ray spectroscopy maps the expelled chemical elements. In Cassiopeia A, the Chandra X-ray Observatory resolves the outer shock and heated debris. Such observations connect an explosion's kinetic energy and newly produced elements to the subsequent heating and enrichment of the interstellar medium.^[ref]