If a hot object (temperature $T_h$) is radiating energy to cooler surroundings (temperature $T_c$) engineers express the radiation heat loss as:
$Q = \sigma \varepsilon (T_h^4 - T_c^4) A$
which is directly derived from the black body law. $A$ is the area of the hot object, $\varepsilon$ its emissivity and $\sigma$ the Stefan-Boltzmann constant.
Even though this equation seems very well established and is really just a slightly modified version of the black body radiation equation, today I tried to apply it to a few common everyday cases and the results don’t make sense. They are impossibly high. The most disturbing case is the heat loss (due to radiation) for a human in an environment at room temperature, that I will derive below.
Let’s say a man ($T_h = 37 \deg = 310 \text{ K}$) stands in a room ($T_c = 20 \deg = 293 \text{ K}$). The surface area of a grown-up person has been estimated to be roughly $2 \text { m}^2$. The diffusivity of human skin is also not very well known but 0.9 seems reasonable. And $\sigma$ is $5.67 \times 10^{-8}$ in S.I. units.
Which gives 0.9*(5.67e-8)*2*((310^4)-(293^4))
, close to 190 W.
That means the heat lost as radiation by an average dude during a single day is $3600 \times 24 \times 190 \approx 16 \text{ MJ}$. That’s around 4000 kcal: food intake is not even close to simply compensating this huge heat loss (not even speaking about the amount spent as mechanical energy or anything). And that’s in a 20 degrees room! Just imagine if he goes outside on a cold winter day...
What’s wrong here?