There is a discussion about the relationship between mass and surface temperature of blue supergiants, particularly a star with 24 solar masses. A rough formula suggests that temperature can be estimated using T = T(sol)*M^0.5, resulting in a calculated temperature of 28,306 K, which is outside the expected range for O-class stars. Factors such as spectral class, luminosity, age, and metal content are considered important in determining a star's surface temperature. The consensus leans towards the idea that there may not be a reliable relationship between mass and temperature for non-main sequence stars. Overall, more information is needed to accurately calculate the surface temperature of such massive stars.