When a Star Runs Out of Fuel

Every star has a beginning, a life span, and an end, and the way a star dies depends largely on its mass. Every star has a beginning, a life span, and an end, and the way a star dies depends largely on its mass. In this book, you will follow the physical processes that shape a star's fate, from the exhaustion of nuclear fuel in its core to the various outcomes that can follow: white dwarfs, neutron stars, supernovae, and black holes. You will learn how stellar remnants influence their surroundings, how the elements formed in dying stars find their way into new generations of stars and planets, and why the study of stellar death remains central to modern astronomy. This book was generated by artificial intelligence and offers a clear, factual introduction to a subject that connects the smallest particles to the largest structures in the universe.