Cited by 280Astro and Planetary ScienceAtmospheric chemistry and aerosolsOrigins and Evolution of Life

Organic haze on Titan and the early Earth

Open access
Trainer, Melissa G., Pavlov, Alexander A., DeWitt, H. Langley, Jimenez, Jose L., McKay, Christopher P., Toon, Owen B., Tolbert, Margaret A.·2006·Proceedings of the National Academy of Sciences

Abstract

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.

Integrity signals

Registry

Crossref · 10.1073/pnas.0608561103

Cites

53 of 53 references verified0 citation errors · 0 not checkable

Statistics

Recomputing p-values needs the paper’s full text.

Claims the paper makes

We couldn’t retrieve this paper’s full text, so its claims and self-check weren’t run. The registry and citation checks still apply.

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • 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]

Cites

Flagged first, then by citations

Cited by

Sorted by citations

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.
Venue
Proceedings of the National Academy of Sciences
Published
2006-11-28
Volume
103
Issue
48
Pages
18035-18042
ISSN
  • 0027-8424 (ISSN-L)
  • 1091-6490
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
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

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review