PHYSICS
Stefan-Boltzmann Law
The law states that the rate of emission of radiant energy per unit area or the power radiated per unit area of a perfect blackbody is directly proportional to the fourth power of its absolute temperature.
The law states that the rate of emission of radiant energy per unit area or the power radiated per unit area of a perfect blackbody is directly proportional to the fourth power of its absolute temperature.
The data that we can put forward from this question is , Length L= 100cm …
The data available in the sums is, Joule mass m = 20g = 0.020kg To find …
The given data from the question can be listed as, mass m = 2kg Total Ener…