Albedo = fraction of incoming light that's reflected.
Using the blackbody approximation and Wien's displacement lawWP, the Sun's emission peak is at 0.5 microns, while the Earth's is at 10 microns, and the comet's is not much different.
The amount of energy absorbed = (1 - albedo) * incoming energy
The amount of energy emitted = (1 - albedo) * blackbody or perfect-emitter limit
Received flux = F
Area of emission = A
Stefan-Boltzmann law = F = A*σ*T4giving Tbb = (F/(A*σ))1/4bb = blackbody or perfect emission and absorption
Taking into account absorption and emission albedos, we get T = Tbb * (1 - aabs)1/4 / (1 - aem)1/4a = albedo
If aem > aabs, then one gets a greenhouse effect.
Using the blackbody approximation and Wien's displacement lawWP, the Sun's emission peak is at 0.5 microns, while the Earth's is at 10 microns, and the comet's is not much different.
The amount of energy absorbed = (1 - albedo) * incoming energy
The amount of energy emitted = (1 - albedo) * blackbody or perfect-emitter limit
Received flux = F
Area of emission = A
Stefan-Boltzmann law = F = A*σ*T4giving Tbb = (F/(A*σ))1/4bb = blackbody or perfect emission and absorption
Taking into account absorption and emission albedos, we get T = Tbb * (1 - aabs)1/4 / (1 - aem)1/4a = albedo
If aem > aabs, then one gets a greenhouse effect.