In modern physics, as it was called "Stefan-Boltzmann law", the total energy radiated per unit surface area of a black body is directly proportional to the fourth power of the black body's temperature T
as:
![P\alpha T^4](https://img.qammunity.org/2020/formulas/physics/high-school/8reutwwjzpgjn84cgnllzpnqksv9tli10i.png)
where: P is the power (total energy radiated per second per square meter) and T is the temperature of a black body.
then we can make a ratio between the state of before quadruple (with subscript 1) and after (with subscript 2) as:
![(P_(1) )/(P_(2) ) =(T_(1)^4 )/(T_(2)^4)](https://img.qammunity.org/2020/formulas/physics/high-school/wezpoca8cbvc415sjb1mvxrdw1r1dhw722.png)
As
![T_(2)=4T_(1)](https://img.qammunity.org/2020/formulas/physics/high-school/59isww3fniwxwbt082j336eozvr9qggwn1.png)
Then
![(P_(1) )/(P_(2) ) =(T_(1)^4 )/((4T_(1))^4)](https://img.qammunity.org/2020/formulas/physics/high-school/71vzw4bxxy0892n9e26gfg0xsik0heum23.png)
then
![P_(2)=256*P_(1)](https://img.qammunity.org/2020/formulas/physics/high-school/yf96kcgcvy5bgknmhf9dwhd4iz154pn1v5.png)
- The factor will the total energy radiated per second per square meter increase = 256