Review the key concepts, formulae, and examples before starting your quiz.
🔑Concepts
The Greenhouse Effect is a process where certain gases in the Earth's atmosphere trap heat, preventing it from escaping into space and keeping the planet warmer than it would be otherwise.
Greenhouse gases (GHGs) include carbon dioxide (), methane (), water vapor (), and nitrous oxide (). These molecules have vibrational modes that resonate at frequencies corresponding to long-wavelength infrared radiation.
Solar radiation is primarily short-wavelength (visible and UV). The Earth absorbs this and re-emits energy as long-wavelength infrared (IR) radiation because the Earth's surface temperature is much lower than the Sun's.
The Albedo () of a body is the ratio of the power of radiation reflected from the body to the total incident power. For Earth, the average albedo is approximately .
The Solar Constant () is the intensity of solar radiation at the top of the Earth's atmosphere, approximately .
Blackbody Radiation: Earth and the Sun are modeled as blackbodies. The Stefan-Boltzmann Law states that the power emitted per unit area is proportional to the fourth power of the absolute temperature ().
Wien's Displacement Law relates the peak wavelength () of emitted radiation to the temperature: .
Energy Balance: For a planet with no atmosphere to be in thermal equilibrium, the power absorbed from the sun must equal the power radiated by the planet: .
📐Formulae
💡Examples
Problem 1:
Calculate the theoretical surface temperature of Earth if it had no atmosphere, given that the solar constant and the average albedo . (Use )
Solution:
The power absorbed per unit area is . Setting this equal to the radiated power :
Explanation:
The factor of accounts for the fact that the Earth intercepts solar radiation as a disk () but radiates it as a sphere (). The resulting temperature of () is much lower than the actual average temperature (), demonstrating the warming effect of the atmosphere.
Problem 2:
Explain why is a greenhouse gas while is not, in terms of molecular resonance.
Solution:
is a homonuclear diatomic molecule with no permanent dipole moment, and its vibrations do not create a changing dipole moment. , while linear and non-polar, has vibrational modes (bending and asymmetrical stretching) that create a transient dipole moment. These modes have natural frequencies in the infrared spectrum.
Explanation:
For a molecule to absorb infrared radiation, the photon's energy must match the difference between vibrational energy levels (), and the vibration must cause a change in the dipole moment of the molecule.