Organic haze on Titan and the early Earth
Open accessAbstract
Recent exploration by the Cassini/Huygens mission has stimulated a great deal of interest in Saturn's moon, Titan. One of Titan's most captivating features is the thick organic haze layer surrounding the moon, believed to be formed from photochemistry high in the CH 4 /N 2 atmosphere. It has been suggested that a similar haze layer may have formed on the early Earth. Here we report laboratory experiments that demonstrate the properties of haze likely to form through photochemistry on Titan and early Earth. We have used a deuterium lamp to initiate particle production in these simulated atmospheres from UV photolysis. Using a unique analysis technique, the aerosol mass spectrometer, we have studied the chemical composition, size, and shape of the particles produced as a function of initial trace gas composition. Our results show that the aerosols produced in the laboratory can serve as analogs for the observed haze in Titan's atmosphere. Experiments performed under possible conditions for early Earth suggest a significant optical depth of haze may have dominated the early Earth's atmosphere. Aerosol size measurements are presented, and implications for the haze layer properties are discussed. We estimate that aerosol production on the early Earth may have been on the order of 10 14 g·year −1 and thus could have served as a primary source of organic material to the surface.
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If the CH4:CO2 ratio exceeds ~0.1 in a UV-irradiated CO2-N2-CH4 mixture, radicals from methane photolysis polymerize into organic particles.
“Empirically, if the CH4:CO2 ratio exceeds ~0.1 in a UV-irradiated CO2-N2-CH4 mixture, radicals from methane photolysis polymerize into organic particles (192).”
From The Archean atmosphere (2020) · cites this paper as [192]
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- Authors
- Trainer, M. G., Pavlov, A. A., DeWitt, H. L., Jimenez, J. L., McKay, C. P., Toon, O. B., & Tolbert, M. A.
- Affiliations
- University of Colorado Boulder (US)
- University of Arizona (US)
- Cooperative Institute for Research in Environmental Sciences (US)
- Ames Research Center (US)
- Corresponding author
- Tolbert, Margaret A.
- ORCID
- Venue
- Proceedings of the National Academy of Sciences
- Publisher
- National Academy of Sciences
- Published
- 2006-11-28
- Volume
- 103
- Issue
- 48
- Pages
- 18035-18042
- ISSN
- 0027-8424 (ISSN-L)
- 1091-6490
- PMC
- PMC1838702
- OpenAlex
- W2018028106
- Cited by
- 280
- References
- 53
- Citations by year
- 2026: 15 · 2025: 22 · 2024: 19 · 2023: 19 · 2022: 14 · 2021: 17 · 2020: 23 · 2019: 18 · 2018: 22 · 2017: 20 · 2016: 6 · 2015: 10 · 2014: 14 · 2013: 22 · 2012: 8
- FWCI
- 2.49
- Type
- journal article
- Language
- en
- Open access
- green
- www.ncbi.nlm.nih.gov
- Locations
- Proceedings of the National Academy of Sciences (publishedVersion)
- Europe PMC (PubMed Central) (publishedVersion)
- PubMed Central (publishedVersion)
- PubMed (publishedVersion)
- Funders
- National Science Foundation
- National Aeronautics and Space Administration (NNG05GA53G, NNG04GM42G)
- John Simon Guggenheim Memorial Foundation
- NASA Astrobiology Institute
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Atmospheric chemistry and aerosols
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Origins and Evolution of Life
- Keywords
- Titan haze, early Earth atmosphere, UV photolysis, aerosol mass spectrometry, optical depth, organic aerosol
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