greenhouse effect

greenhouse effect

The greenhouse effect is the process in which greenhouse gases in the atmosphere of a planet or moon transmit radiant energy from the host star but are opaque to the longer wavelengths of infrared radiation, or heat, which re-radiate from the surface. This results in an elevation of the surface temperature. The Earth, for example, is about 35°C warmer overall than it would be without any greenhouse contribution, while the runaway greenhouse effect on Venus pushes up the surface temperature there by as much as 500°C. By contrast, the thin carbon dioxide atmosphere on Mars contributes only about a 5°C rise in surface temperature.


How the greenhouse effect works

The greenhouse effect can be explained with the aid of Wein's displacement law. This states that the wavelength at which a blackbody radiates most intensely varies inversely with its absolute temperature. Thus the radiation originating in the hot sun is of much shorter wavelength than that radiated from the cool Earth or its atmosphere. Since the atmosphere, particularly when laden with water vapor, is far more opaque to the long-wavelength radiation characteristic of the Earth than it is to incoming solar radiation, it tends to absorb the former radiation and reradiates it, largely back toward the surface, ensuring that the Earth's surface is maintained at a somewhat higher temperature than would be the case were all the energy radiated from the surface lost directly into space. Actually, less than half the short-wave solar radiation arriving at the top of the atmosphere is absorbed at the Earth's surface. Much is scattered into space by minute particles in the atmosphere or absorbed by atmospheric dust, ozone, carbon dioxide, and water vapor. This last, absorbed energy becomes involved in the long-wavelength radiation processes. Some energy is transferred from the surface to the atmosphere by convection and as latent heat of vaporization of water.