The Stefan-Boltzmann Law states that the total energy output…

The Stefan-Boltzmann Law states that the total energy output of a blackbody is proportional to the surface temperature to the fourth power: E = σT4 . If you have a star that is at double the temperature of our Sun, the total energy output of that star would be

The Stefan-Boltzmann Law states that the total energy output…

The Stefan-Boltzmann Law states that the total energy output of a blackbody is proportional to the surface temperature to the fourth power: E = σT4 . If you have a star that is at double the temperature of our Sun, the total energy output of that star would be