Literature DB >> 11538492

The greenhouse and antigreenhouse effects on Titan.

C P McKay1, J B Pollack, R Courtin.   

Abstract

There are many parallels between the atmospheric thermal structure of the Saturnian satellite Titan and the terrestrial greenhouse effect; these parallels provide a comparison for theories of the heat balance of Earth. Titan's atmosphere has a greenhouse effect caused primarily by pressure-induced opacity of N2, CH4, and H2. H2 is a key absorber because it is primarily responsible for the absorption in the wave number 400 to 600 cm-1 "window" region of Titan's infrared spectrum. The concentration of CH4, also an important absorber, is set by the saturation vapor pressure and hence is dependent on temperature. In this respect there is a similarity between the role of H2 and CH4 on Titan and that of CO2 and H2O on Earth. Titan also has an antigreenhouse effect that results from the presence of a high-altitude haze layer that is absorbing at solar wavelengths but transparent in the thermal infrared. The antigreenhouse effect on Titan reduces the surface temperature by 9 K whereas the greenhouse effect increases it by 21 K. The net effect is that the surface temperature (94 K) is 12 K warmer than the effective temperature (82 K). If the haze layer were removed, the antigreenhouse effect would be greatly reduced, the greenhouse effect would become even stronger, and the surface temperature would rise by over 20 K.

Entities:  

Keywords:  NASA Center ARC; NASA Discipline Exobiology; NASA Discipline Number 52-50; NASA Program Exobiology

Mesh:

Substances:

Year:  1991        PMID: 11538492     DOI: 10.1126/science.11538492

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  8 in total

1.  The two-box model of climate: limitations and applications to planetary habitability and maximum entropy production studies.

Authors:  Ralph D Lorenz
Journal:  Philos Trans R Soc Lond B Biol Sci       Date:  2010-05-12       Impact factor: 6.237

2.  A coupled ecosystem-climate model for predicting the methane concentration in the Archean atmosphere.

Authors:  J F Kasting; A A Pavlov; J L Siefert
Journal:  Orig Life Evol Biosph       Date:  2001-06       Impact factor: 1.950

Review 3.  Chemical evolution on Titan: comparisons to the prebiotic earth.

Authors:  D W Clarke; J P Ferris
Journal:  Orig Life Evol Biosph       Date:  1997-06       Impact factor: 1.950

4.  Earth's outgoing longwave radiation linear due to H2O greenhouse effect.

Authors:  Daniel D B Koll; Timothy W Cronin
Journal:  Proc Natl Acad Sci U S A       Date:  2018-09-25       Impact factor: 11.205

5.  Rovibrational energy and spectroscopic constant calculations of CH4⋯CH4, CH4⋯H2O, CH4⋯CHF3, and H2O⋯CHF3 dimers.

Authors:  Wiliam F Cunha; Ricardo Gargano; Edgardo Garcia; José R S Politi; Alessandra F Albernaz; João B L Martins
Journal:  J Mol Model       Date:  2014-06-18       Impact factor: 1.810

6.  Atmospheric composition and climate on the early Earth.

Authors:  James F Kasting; M Tazewell Howard
Journal:  Philos Trans R Soc Lond B Biol Sci       Date:  2006-10-29       Impact factor: 6.237

7.  Dimming titan revealed by the Cassini observations.

Authors:  Liming Li
Journal:  Sci Rep       Date:  2015-02-04       Impact factor: 4.379

8.  Titan as the Abode of Life.

Authors:  Christopher P McKay
Journal:  Life (Basel)       Date:  2016-02-03
  8 in total

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