F Dwarfs are a type of star classified by their surface temperature and brightness. They are part of the Hertzsprung-Russell diagram, which categorizes stars based on their luminosity and temperature. F Dwarfs have temperatures ranging from about 6,000 to 7,600 degrees Celsius and are typically yellow-white in color. They are more massive than G Dwarfs, like our Sun, and can be found in various stages of their life cycle. These stars are known for their stability and can have lifespans of several billion years. F Dwarfs often host planetary systems, making them interesting targets for the search for exoplanets. Their characteristics make them valuable for studying stellar evolution and the potential for life in the universe.