White dwarfs, the last step in the evolution of stars like our Sun, are tiny, blue compact objects, with a mass comparable to that of the Sun but packed into the size of a planet—or even smaller—a moon! Although very common (more than 95% of all stars are destined to become white dwarfs), these incredibly dense remnants still hide many secrets and mysteries. Dr. Caiazzo will discuss how a small old telescope at the Palomar Observatory, refurbished with a brand new instrument, ZTF, is allowing researchers to discover white dwarfs with extreme properties like huge magnetic fields and rapid rotation speeds—including the smallest white dwarf known. These discoveries are challenging our understanding of white dwarf evolution, as well as leading to new insights into the connection between white dwarfs and supernovae.
