B-Type Stars are a class of hot, massive stars characterized by their blue-white color and high temperatures, typically ranging from 10,000 to 30,000 Kelvin. They are often much larger than our Sun, with masses between 2.1 and 16 times that of the Sun. Due to their size and temperature, B-type stars have short lifespans, usually only a few million years. These stars are known for their strong stellar winds and significant ultraviolet radiation, which can influence their surrounding environments. B-Type Stars are often found in young star clusters and play a crucial role in the chemical evolution of galaxies by enriching the interstellar medium with heavier elements when they explode as supernovae.