The solar system was formed from ejected matter from supernovae, but pinpointing the exact remnants of these events, such as black holes or neutron stars, is highly challenging due to the system's age and the complex dynamics of stellar orbits. Heavy elements in our solar system likely originated from multiple supernovae, with one supernova believed to have made the most significant contribution. Over 4.5 billion years, the solar system has orbited the galaxy about twenty times, complicating the search for remnants that may have drifted away. While some remnants may still exist, their high velocities and potential ejection from the galaxy make them difficult to locate. Future discoveries may identify candidates related to our solar system's formation, but current evidence remains speculative.