Astrophysics (Index)About

greenhouse effect

(mechanism that boosts temperature through selective blocking of EMR)

The term greenhouse effect is used for atmospheres, referring to the same mechanism by which greenhouses can remain warmer than surrounding air, i.e., that the energy carried in by incoming electromagnetic radiation (EMR) is not efficiently carried out by outgoing EMR. The imbalance leads to energy gathering in the form of heat, the temperature rising to the point that it produces sufficient EMR emission to reach a balance. In the case of a greenhouse, the effect is because of the glass's differing transparency at different wavelengths, whereas for a planet, the effect is due to such differing transparency of the atmosphere. In both cases, this varying transparency is easily measured and is necessarily taken into account for much technology (atmospheric windows) and the effect is easily produced in lab experiments. (If this seems strange, note that EMR in the form of radio waves passes right through many walls that block light waves.)

The Earth's temperature is in part maintained by a greenhouse effect, due to the atmosphere's efficient transmission of much of the Sun's visible light down to the surface, and its opacity in some infrared wavelengths, which is what would carry away the bulk of the energy given the Earth's temperature. The components of the atmosphere that block EMR are known as greenhouse gases. Changes in the atmosphere's makeup would affect the greenhouse effect, such as the addition of greenhouse gases causing the Earth's surface temperature to rise. In fact, the ever-increasing use of technology that burns fossil fuels is adding a greenhouse gas (carbon dioxide). There is much current political interest in whether a resulting rise in the global temperature has been detected and what polices and practices should be our response.

Runaway greenhouse effect occurs in cases where a rising temperature increases the presence of greenhouse gases, which in turn raise the temperature, i.e., positive feedback, resulting in a large rise in temperature. An example of such a runaway greenhouse effect might be a rise in temperature causing an increase in water vapor (a greenhouse gas) in the atmosphere, i.e., if the warming of surface-water (oceans) caused sufficient additional water to evaporate into the atmosphere to increase the temperature, further warming the surface-water, causing more such evaporation, etc.

A moist greenhouse effect is one possible scenario for Earth, consisting of the Earth atmosphere's cold trap no longer preventing water vapor from reaching the upper atmosphere. Water vapor above the cold trap would undergo slow photodissociation, and would slowly be replenished from below. The resulting hydrogen would escape the atmosphere, and Earth's water would be gradually eliminated.

The greenhouse effect affects other worlds to varying degrees: Venus has a temperature of 730 K (about 850°F) whereas without the greenhouse effect, its temperature would be roughly the equilibrium temperature, 328 K (about 160°F). Earth's, in contrast, raises the temperature on the order of 10°F, and the difference is apparently that in Venus's history, a runaway greenhouse effect occurred.

The analysis of extra-solar planet and solar system planet and moon atmospheres and temperature must take the effect into account.


(EMR,physics,temperature,exoplanets)
Further reading:
https://en.wikipedia.org/wiki/Greenhouse_effect
https://en.wikipedia.org/wiki/Greenhouse_gas
https://en.wikipedia.org/wiki/Runaway_greenhouse_effect
https://en.wikipedia.org/wiki/Runaway_greenhouse_effect#The_moist_greenhouse_limit
https://climate.nasa.gov/faq/19/what-is-the-greenhouse-effect/
https://www.britannica.com/science/greenhouse-effect
https://scied.ucar.edu/learning-zone/how-climate-works/greenhouse-effect
https://climate.mit.edu/explainers/greenhouse-gases
https://www.esa.int/Science_Exploration/Space_Science/Venus_Express/Greenhouse_effects_also_on_other_planets

Referenced by pages:
atmospheric window
carbon dioxide (CO2)
equilibrium temperature (Teq)
faint young Sun paradox
line blanketing
Mars
radiative forcing (RF)
runaway process
silicate weathering feedback
thermal runaway
Venus

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