A steel spoon in hot tea becomes hot, a room heater warms the air above it, and the Sun warms the Earth across empty space. In this course we study conduction with the thermal conductivity, convection, and radiation with the laws of Stefan and Wien, and Newton's law of cooling, which tells us how fast a hot body cools.
3 lessons, about 1 h 15 min3 simulations12 problems6 practice questionsPython in every lesson
In conduction, heat passes through a material from particle to particle, without the material moving. Through a slab in steady state, , where is the thermal conductivity: copper , glass , wool . A slab's thermal resistance is , and layers add their resistances.
In convection, a warmed fluid rises and carries heat with it, as in sea breezes and boiling pans. Radiation is heat carried by electromagnetic waves, even through a vacuum. A body at radiates (Stefan's law), most strongly at (Wien's law); good absorbers are good emitters.
For a small difference of temperature, a body cools at a rate in proportion to its excess over its surroundings: . The excess then falls exponentially, , quickly at first and slowly later. Over a short interval, the average excess gives a quick estimate.
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