Potential climatic impact of organic haze on early earth

Christa A. Hasenkopf, Miriam A. Freedman, Melinda R. Beaver, Owen B. Toon, Margaret A. Tolbert

Research output: Contribution to journalArticle

14 Citations (Scopus)

Abstract

We have explored the direct and indirect radiative effects on climate of organic particles likely to have been present on early Earth by measuring their hygroscopicity and cloud nucleating ability. The early Earth analog aerosol particles were generated via ultraviolet photolysis of an early Earth analog gas mixture, which was designed to mimic possible atmospheric conditions before the rise of oxygen. An analog aerosol for the present-day atmosphere of Saturn's moon Titan was tested for comparison. We exposed the early Earth aerosol to a range of relative humidities (RHs). Water uptake onto the aerosol was observed to occur over the entire RH range tested (RH=80-87%). To translate our measurements of hygroscopicity over a specific range of RHs into their water uptake ability at any RH < 100% and into their ability to act as cloud condensation nuclei (CCN) at RH > 100%, we relied on the hygroscopicity parameter κ, developed by Petters and Kreidenweis. We retrieved κ=0.22±0.12 for the early Earth aerosol, which indicates that the humidified aerosol (RH < 100 %) could have contributed to a larger antigreenhouse effect on the early Earth atmosphere than previously modeled with dry aerosol. Such effects would have been of significance in regions where the humidity was larger than 50%, because such high humidities are needed for significant amounts of water to be on the aerosol. Additionally, Earth organic aerosol particles could have activated into CCN at reasonable-and even low-water-vapor supersaturations (RH > 100%). In regions where the haze was dominant, it is expected that low particle concentrations, once activated into cloud droplets, would have created short-lived, optically thin clouds. Such clouds, if predominant on early Earth, would have had a lower albedo than clouds today, thereby warming the planet relative to current-day clouds.

Original languageEnglish (US)
Pages (from-to)135-149
Number of pages15
JournalAstrobiology
Volume11
Issue number2
DOIs
StatePublished - Mar 1 2011

Fingerprint

early Earth
haze
aerosols
Humidity
Aerosols
humidity
relative humidity
hygroscopicity
aerosol
Wettability
Earth analogs
Saturn
water uptake
Planets
Water
Titan
Photolysis
photolysis
cloud droplet
natural satellites

All Science Journal Classification (ASJC) codes

  • Agricultural and Biological Sciences (miscellaneous)
  • Space and Planetary Science

Cite this

Hasenkopf, C. A., Freedman, M. A., Beaver, M. R., Toon, O. B., & Tolbert, M. A. (2011). Potential climatic impact of organic haze on early earth. Astrobiology, 11(2), 135-149. https://doi.org/10.1089/ast.2010.0541
Hasenkopf, Christa A. ; Freedman, Miriam A. ; Beaver, Melinda R. ; Toon, Owen B. ; Tolbert, Margaret A. / Potential climatic impact of organic haze on early earth. In: Astrobiology. 2011 ; Vol. 11, No. 2. pp. 135-149.
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Hasenkopf, CA, Freedman, MA, Beaver, MR, Toon, OB & Tolbert, MA 2011, 'Potential climatic impact of organic haze on early earth', Astrobiology, vol. 11, no. 2, pp. 135-149. https://doi.org/10.1089/ast.2010.0541

Potential climatic impact of organic haze on early earth. / Hasenkopf, Christa A.; Freedman, Miriam A.; Beaver, Melinda R.; Toon, Owen B.; Tolbert, Margaret A.

In: Astrobiology, Vol. 11, No. 2, 01.03.2011, p. 135-149.

Research output: Contribution to journalArticle

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