The sun is expected to transition to a black dwarf in a timeframe exceeding one trillion years, with estimates suggesting it could take around two trillion years to cool below 800 K. The cooling process is influenced by weakly interacting massive particles (WIMPs), which may keep some white dwarfs warmer for up to 10^25 years. Current models indicate that a white dwarf, starting at approximately 4000 K, will take significantly longer to reach a state where it no longer emits visible heat. The presence of an opaque outer crust on white dwarfs slows down heat escape, affecting cooling rates. Ultimately, the transition to a black dwarf is a complex process dependent on various factors.