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This code (ThermalEvolution1D.cpp) models the thermal evolution of small planetary bodies, particularly icy moons. I solve the 1-D heat diffusion equation assuming only conduction. Heat sources include short- and long-lived radioactive isotopes and tidal heating. Heat sinks include silicate dehydration.
ktrinh20/ThermalEvolution1D
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This code (ThermalEvolution1D.cpp) models the thermal evolution of small planetary bodies, particularly icy moons. I solve the 1-D heat diffusion equation assuming only conduction. Heat sources include short- and long-lived radioactive isotopes and tidal heating. Heat sinks include silicate dehydration.
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