Evidence map›Paper›PMID 17101962›Full record

ArticleProceedings of the National Academy of Sciences of the United States of America2006

Organic haze on Titan and the early Earth.

Melissa G Trainer, Alexander A Pavlov, H Langley DeWitt, Jose L Jimenez, Christopher P McKay, Owen B Toon, Margaret A Tolbert

Abstract read
In one paragraph

Article in Proceedings of the National Academy of Sciences of the United States of America, 2006. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 32 papers.

0numbers the graph read from it
0cells of the map it votes in
32citing papers in PubMed
2.9field-weighted citation impact, top 10% of its field
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

32 citing papers in PubMed, 259 citations in OpenAlex.

  1. Abiotic CONature communications · 2026
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  2. Review
  3. Article
  4. Article
  5. An Archean atmosphere rich in sulfur biomolecules.Proceedings of the National Academy of Sciences of the United States of America · 2025
    Article
  6. Article
  7. Article
  8. Article
  9. Reactant Discovery with anACS earth & space chemistry · 2024
    Article
  10. The Composition and Chemistry of Titan's Atmosphere.ACS earth & space chemistry · 2024
    Review
  11. Article
  12. Article
  13. The Archean atmosphere.Science advances · 2020
    Review
  14. Review
  15. Review
  16. Constraining the climate and ocean pH of the early Earth with a geological carbon cycle model.Proceedings of the National Academy of Sciences of the United States of America · 2018
    Article
  17. Article
  18. Article
  19. Article
  20. Biological regulation of atmospheric chemistry en route to planetary oxygenation.Proceedings of the National Academy of Sciences of the United States of America · 2017
    Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

7 authors at 4 institutions in 1 country.

Melissa G TrainerLaboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80309, USA.
Alexander A Pavlov
H Langley DeWitt
Jose L Jimenez
Christopher P McKay
Owen B Toon
Margaret A Tolbert
Cooperative Institute for Research in Environmental Sciences · USLaboratory for Atmospheric and Space Physics · USAmes Research Center · USUniversity of Arizona · US

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

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.

Identifiers

PMID17101962
PMCPMC1838702
OpenAlexW2018028106

What OpenQuestion holds

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Registered trials

None linked

Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.