 Here we see interacting butterfly galaxies, NGC 4567 and 68, located 59 million light years away. In April 2020, the Zwicky Transient Facility at the Palomar Observatory in San Diego discovered a supernova now called SN-2020FQV. At the same time, it turned out that the Transiting Exoplanet Survey Satellite, a NASA satellite designed primarily to discover exoplanets, was looking at the same area of space. The Hubble team was alerted and within hours it had the Hubble telescope focused on the expanding circumstellar material around the exploding star. The team looked at Hubble observations of the star going back to the 1990s. The Exoplanet Survey Satellite provided an image of the system every 30 minutes starting several days before the explosion, through the explosion itself and continuing for weeks. And from studying the circumstellar material with Hubble, the scientists gained an understanding of what was happening around the star over the previous decade. By combining all of this information, the team was able to create a multi-decade look at the star's final years.