Blog Post Image: Confirmed: Stellar Behemoth Self-Destructs in a Type IIb Supernova

A detailed study of the spectrum (the distribution of colors composing the light from the supernova) using a technique called “flash spectroscopy” revealed the signature of a wind blown by the aging star just prior to its terminal explosion, and allowed scientists to determine what elements were abundant on the surface of the dying star as it was about to explode as a supernova, providing important information about how massive stars evolve just prior to their death, and the origin of crucial elements such as carbon, nitrogen and oxygen. Image credit: Berkeley Lab