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Planetary radiative equilibrium
•Energy absorbed = Energy radiated
\(L/(4pd2))pr2 = 4pr2sT4
\T = 278 (L€/d2AU)1/4 K
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•Greenhouse effect :
•    Earth’s atmosphere relatively transparent to solar  radiation (heating) •but re-radiation (cooling) in infrared is impeded (photons absorbed by CO2, H2O)
•For Venus, greenhouse effect is enormous
•due to CO2, T = 600K  (could happen at Earth)
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