A blackbody radiant heating panel of 5 m\(^2\) surface area at 35\(^\circ\)C surface temperature is located 1 m away from a 1 m\(^2\) surface at 20\(^\circ\)C. The Stefan-Boltzmann constant is \(5.6703 \times 10^{-8}\ \text{W m}^{-2} \text{K}^{-4}\). The rate of radiant heat emission by the radiant heating panel (in W, rounded off to two decimal places) is \(\underline{\hspace{2cm}}\).
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Always convert temperatures to Kelvin before using the Stefan–Boltzmann law.