A surface of area loses by convection (coefficient ) plus radiation (emissivity , Stefan-Boltzmann constant ) to surroundings at . Solve
for the surface temperature in kelvin.
Collapse the constants into two coefficients. Group the convection and radiation factors:
so the equation is
Expand into a quartic in standard form. With , the two constant contributions are and :
Do not stop at the linear estimate — this is the trap. Ignoring the quartic term gives
but substituting that back shows why it fails: , six times the entire heat load. The radiation term is dominant at that temperature, not negligible, so is far too high.
Solve the quartic numerically instead. The left-hand side is strictly increasing in for (both and increase), so there is exactly one physical root and bisection converges reliably. Bracketing between and and bisecting gives
Check the root by splitting the two loss mechanisms. At :
and , matching the required heat loss. Radiation carries of the load — confirming it could never have been dropped.
State the answer with its physical reading.
The general lesson: whenever a balance mixes a linear convection term with a radiation term, the quartic must be solved, because radiation grows so steeply that it overtakes convection well before a few hundred kelvin of overtemperature.
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