F-Type Main Sequence Stars
F-Type Main Sequence Stars are a category of stars that are slightly hotter and more massive than the Sun. They have surface temperatures ranging from about 6,000 to 7,500 degrees Celsius. These stars typically have a yellow-white color and are known for their strong hydrogen fusion in their cores, which allows them to shine brightly for billions of years.
These stars are classified as part of the Hertzsprung-Russell diagram, which categorizes stars based on their luminosity and temperature. F-Type stars are often found in binary systems and can host exoplanets, making them of interest in the search for extraterrestrial life.