∆TMantle Heating 1026 K B17 CMantle 1124 Jkg –1K –1 1 MLunar Mantle 6.62E+22 kg 1.B19 ∆HMantle Heating = CM∆TMHMLM 7.63E+28 J Result Table 7 - Energy Requirements to Heat Mantle Parameter Amount Units Ref Boltzmann Constant - kB 1.38E-23 J/K 12 Planck Constant - h 6.63E-34 Js 13 Speed of Light - c 3.00E+08 m/s 14 Stefan-Boltzmann - σ = 2π5k B 4/(15h3c2) 5.67E-08 Jm–2s–1K –1 15 Overall Lunar Radius - RO 1.74E+06 m 1.B4 Lunar Surface Area - AL = 4πRO 2 3.79E+13 m2 Fraction of Surface Covered by Lava - FSCL 30% m2/m2 Trial Atomisation Area Increase Factor - FAAI 500% m2/m2 Trial Effective Radiating Area - AE = ALFSCLFAAI 5.69E+13 m2 Trial Surface Temperature - TS 2998 K B40 Maximum Radiated Power - PM = σAETS 4 2.61E+20 W 16 Timescale for Radiation - tR (1 year) 3.16E+07 s Flood Radiated Energy Estimate - ∆HR = PMtR 8.23E+27 J Result Table 6 - Radiation Heat Loss STERNBERG Craters and cracks 2023 ICC 45
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