Use the Stefan-Boltzmann law: heat gained =
q =A σ (ε T14 - φT24)
where σ=5.669E-8 W/m2/K4 is Boltzmann's constant, A is the surface area of the absorbing surface and φ and T2 its absorptivity and temperature, and ε and T1 are the emissivity and temperature of the radiating surface. In this case, the radiating surface is a blackbody, so ε=1. The temperatures are T1=1000 °C = 1273 K and T2=100 °C = 373 K. You get
q = 0.15 m2 (5.669E-8 W/m2/K4) (1*12734 - 0.8*3734)K4 = 22,200 W.