According to Stefan-Boltzmann law, the energy radiated per unit area per second by a body is proportional to:
T⁴
The Stefan-Boltzmann law states that the total energy radiated per unit area per second (the emissive power) by a black body is directly proportional to the fourth power of its absolute temperature:
\(E = \sigma T^{4}\)
where \(\sigma\) is the Stefan-Boltzmann constant. So the energy radiated is proportional to \(T^{4}\), not to \(T\), \(T^{2}\), or \(T^{3}\).
Important Questions from Heat and Transfer
The brightness of a star depends on its
Thermocouple is a device which converts
To change a temperature on the Kelvin scale to the Celsius scale, you have to ________ the given temperature.
Ramu mixes 2 litres of water at 100°C and 18 litres of water at 32°C. What temperature will the water have after mixing?
Which one of the following is the correct relation between the Kelvin temperature (T) and the Celsius temperature (tc)?
