Yes, in principle, but only if their emissivity is independent of temperature. Generally, emissivity is a very weak function of temperature.
The radiating power changes by a factor of 16 when the absolute temperature of a radiator is doubled. This is because the radiating power is proportional to the fourth power of the absolute temperature according to the Stefan-Boltzmann law.
The total energy radiated by a blackbody increases with temperature according to Stefan-Boltzmann law, which states that the total power radiated per unit area is proportional to the fourth power of the absolute temperature. This means that as the temperature of a blackbody increases, the total energy it radiates also increases significantly.
Fluorescent light bulbs are typically more energy-efficient and produce more light for the same amount of power compared to incandescent bulbs. So, a fluorescent light bulb may appear brighter than an incandescent bulb with the same power rating.
The total energy radiated by a blackbody is directly proportional to the fourth power of its temperature, as described by the Stefan-Boltzmann law. This means that as the temperature of the blackbody increases, the amount of energy it radiates also increases rapidly.
The heat energy radiated by a body increases with the temperature raised to the fourth power according to the Stefan-Boltzmann law. This means that as the temperature of a body increases, the amount of heat energy radiated also increases significantly.
Incandescent lamps are nearly pure resistive loads with a power factor of 1
Two to the fourth power times 5 to the fourth power equals 10,000
The answer to 200 to the fourth power is 1,600,000,000
No, it is not.
3 to the fourth power=81Three to the fourth power is 81.
m4n4
0.6 to the fourth power equals 0.1296
-3 to the fourth power = 81
The radiating power changes by a factor of 16 when the absolute temperature of a radiator is doubled. This is because the radiating power is proportional to the fourth power of the absolute temperature according to the Stefan-Boltzmann law.
± 2.632148 to the fourth power equals 48.
The Answer is 656
The luminosity of a star is proportional to the fourth power of its temperature. Since the total flux has increased by a factor of 625, the temperature of the star would increase by the fourth root of 625, which is 5. Therefore, the temperature of the star would have increased by a factor of 5.