According to Stefan-Boltzmann law, the total energy radiated
per unit area of a block body is directly proportional to the fourth power of
the black body’s temperature T i.e.
j=σT4
Where, σ is constant of proportionality called as Stefan–Boltzmann constant
Case 1.
T1=7270C=1000K
So, E=σ×(1000)4..............(1)
Case 2
T2=22270C=2500K
E′=σ×(2500)4.....(2)
Taking ratio of (1) and (2)
EE′=σ×(1000)4σ×(2500)4
EE′=16625
625E16=E′
The energy increases by a factor of 625E16.