The universe is filled with powerful explosions that help scientists understand how stars live, evolve, and die. Among the most important of these events are Type Ia supernovae, incredibly energetic stellar explosions that play a major role in the evolution of galaxies and the formation of chemical elements. For decades, astronomers have investigated how these explosions begin. One leading explanation involves two white dwarfs, the dense remains of stars that have reached the end of their lives. Now, researchers have identified a remarkable pair of white dwarfs whose combined mass exceeds a critical limit known as the Chandrasekhar limit. This discovery could help scientists understand how some of the universe's most important stellar explosions occur. The system, named WDJ181058.67+311940.94 , is particularly interesting because it is relatively close to Earth and may eventually produce a Type Ia supernova. What Are White Dwarfs? White dwarfs are the small, extremely dense remains...