Runaway greenhouse effect

A runaway greenhouse effect is not a clearly defined term, but is understood to mean an event analogous to that which is believed to have happened in the early history of Venus, where positive feedback increased the strength of its greenhouse effect until its oceans boiled away.[1][2] The term is not generally used by the IPCC, which in one of its few mentions says a “runaway greenhouse effect” — analogous to Venus - appears to have virtually no chance of being induced by anthropogenic activities.[3]

Other, less catastrophic events, may loosely be called a "runaway greenhouse". It has been hypothesised that such may have occurred at the Permian-Triassic extinction event.[4][5] Terrestrial climatologists often use the term 'abrupt', rather than 'runaway', when describing such scenarios.[6]

Contents

Feedbacks

Positive feedbacks do not have to lead to a runaway effect, as the gain is not always sufficient. Radiation from a planet increasing in proportion to the fourth power of temperature, in accordance with the Stefan-Boltzmann law, provides a negative feedback; so the positive feedback effect has to be very strong to cause a runaway effect (see gain). An increase in temperature from greenhouse gases leading to increased water vapor which is a greenhouse gas causing further warming is a positive feedback. This is not a runaway effect on Earth.[7] Positive feedback effects are common and always exist (e.g. ice-albedo feedback) while runaway effects are much rarer and cannot be operating at all times.

Venus

A runaway greenhouse effect involving CO2 and water vapor may have occurred on Venus.[8] In this scenario, early Venus may have had a global ocean. As the brightness of the early Sun increased, the amount of water vapor in the atmosphere increased, increasing the temperature and consequently increasing the evaporation of the ocean, leading eventually to the situation in which the oceans boiled, and all of the water vapor entered the atmosphere. On Venus today there is little water vapor in the atmosphere. If water vapor did contribute to the warmth of Venus at one time, this water is thought to have escaped to space. Venus is sufficiently strongly heated by the Sun that water vapor can rise much higher in the atmosphere and be split into hydrogen and oxygen by ultraviolet light. The hydrogen can then escape from the atmosphere and the oxygen recombines. Carbon dioxide, the dominant greenhouse gas in the current Venusian atmosphere, likely owes its larger concentration to the weakness of carbon recycling as compared to Earth, where the carbon dioxide emitted from volcanoes is efficiently subducted into the Earth by plate tectonics on geologic time scales.[9]

Earth

The situation on Earth is very different from that which existed on Venus, as any terrestrial runaway effect is not irreversible on geological timescales. Potential runaway greenhouse effects on Earth may involve the carbon cycle, but unlike Venus will not involve boiling of the oceans. Earth's climate has swung repeatedly between warm periods and ice ages during its history. In the current climate the gain of the positive feedback effect from evaporating water is well below that which is required to boil away the oceans.[10] Climate scientist John Houghton has written that "[there] is no possibility of [Venus's] runaway greenhouse conditions occurring on the Earth".[11]

Benton and Twitchett's have a different definition of a runaway greenhouse;[4] events meeting this definition have been suggested as a cause for the Paleocene-Eocene Thermal Maximum and the great dying.

See also

References

  1. ^ Rasool, I.; De Bergh, C.; De Bergh, C. (Jun 1970). "The Runaway Greenhouse and the Accumulation of CO2 in the Venus Atmosphere". Nature 226 (5250): 1037–1039. Bibcode 1970Natur.226.1037R. doi:10.1038/2261037a0. ISSN 0028-0836. PMID 16057644. http://pubs.giss.nasa.gov/docs/1970/1970_Rasool_DeBergh.pdf. Retrieved 02/25/2009.  hello edit
  2. ^ Dept. Physics & Astronomy. "A Runaway Greenhouse Effect". Univ. of Tenn.. http://csep10.phys.utk.edu/astr161/lect/venus/greenhouse.html. Retrieved 24 July 2010. 
  3. ^ http://www.ipcc.ch/meetings/session31/inf3.pdf
  4. ^ a b Benton, M. J.; Twitchet, R. J. (2003). "How to kill (almost) all life: the end-Permian extinction event". Trends in Ecology & Evolution 18 (7): 358–365. doi:10.1016/S0169-5347(03)00093-4. http://palaeo.gly.bris.ac.uk/Benton/reprints/2003TREEPTr.pdf.  edit
  5. ^ Morante, Richard (1996). "Permian and early Triassic isotopic records of carbon and strontium in Australia and a scenario of events about the Permian-Triassic boundary". Historical Biology: an International Journal of Paleobiology 11 (1): 289–310. http://www.informaworld.com/smpp/951243416-91983953/content~db=all~content=a907603935. 
  6. ^ Kennett, James; Kevin G. Cannariato, Ingrid L. Hendy, and Richard J. Behl. Methane Hydrates in Quaternary Climate Change: The Clathrate Gun Hypothesis. ISBN 0-87590-296-0. 
  7. ^ Kasting, J. F. (1988). "Runaway and moist greenhouse atmospheres and the evolution of Earth and Venus". Icarus 74 (3): 472–494. Bibcode 1988Icar...74..472K. doi:10.1016/0019-1035(88)90116-9. PMID 11538226.  edit
  8. ^ S. I. Rasoonl and C. de Bergh (1970). "The Runaway Greenhouse Effect and the Accumulation of CO2 in the Atmosphere of Venus". Nature 226 (5250): 1037–1039. Bibcode 1970Natur.226.1037R. doi:10.1038/2261037a0. PMID 16057644. 
  9. ^ Nick Strobel. "Venus". http://home.case.edu/~sjr16/venus.html. Retrieved 17 February 2009. 
  10. ^ Isaac M. Held and Brian J. Soden (November 2000). "Water Vapor Feedback and Global Warming". Annual Review of Energy and the Environment 25 (1): 441–475. doi:10.1146/annurev.energy.25.1.441. "On this basis, one might expect runaway conditions to develop eventually if the climate warms sufficiently. Although it is difficult to be quantitative, primarily because of uncertainties in cloud prediction, it is clear that this point is only achieved for temperatures that are far warmer than any relevant for the global warming debate" 
  11. ^ Houghton, J. (May 4, 2005). "Global Warming". Rep. Prog. Phys. 68 (6): 1343–1403. Bibcode 2005RPPh...68.1343H. doi:10.1088/0034-4885/68/6/R02. http://www.iop.org/EJ/abstract/0034-4885/68/6/R02/. Retrieved August 26, 2009.