Question
Derive Newton's law of cooling from Stefan-Boltzman law.

Answer

For a non-black body at temperature T surrounded by an enclosure $T_0$ (where $T > T_0$), we have $\text{E}=\text{e}\sigma(\text{T}^4-\text{T}^4_0)$ where e is a constant, and its value depends upon the physical nature of the emitting surface.
$\therefore\text{E}=\text{e}\sigma(\text{T}^2+\text{T}^2_0)(\text{T}^2-\text{T}_0^2)$ $=\text{e}\sigma(\text{T}^2+\text{T}^2_0)(\text{T}+\text{T}_0)(\text{T}-\text{T}_0)$

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