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 given can be listed as mass of earth , m = 6 x 10²⁴ kg. distance bet…
we can list out the given as, Power P= 100W current , I = 3A To find , R…
the given can be listed as Power P = 100W To Find , Resistance R = ? …