Is OSSO a Significant Contributor to the Unknown UV Absorber in Venus' Atmosphere?

Abstract It has been proposed that two isomers of the SO dimer ( cis ‐ and trans ‐OSSO) are candidates for the unknown UV absorber in Venus' atmosphere because they have a good spectral match with the absorber, despite the low concentrations predicted by 1D photochemical models. Here OSSO chemistry (production from SO and loss by photolysis, thermal decomposition, and reaction with O and Cl) has been included in the photochemistry scheme of a 3D planetary climate model (PCM‐Venus) along with sulfur injection due to meteoric ablation. 1D multiple scattering radiative transfer modeling is then used to predict the resulting top‐of‐the‐atmosphere reflectance produced by OSSO. The modeled OSSO concentrations are shown to be ∼3 orders of magnitude too low to explain the observed absorbance levels, and the predicted ratio of the OSSO isomers provides an unsatisfactory match to the spectral shape of the unknown absorber.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-02-12
DOI
https://doi.org/10.1029/2024gl113090
Citations
3
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
3.46

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article

Is OSSO a Significant Contributor to the Unknown UV Absorber in Venus' Atmosphere?

Joanna Victoria Egan, D. R. Marsh, J. M. C. Plane, Alexander D. James et al.
3 citations
Geophysical Research Letters
Planetary Science and Exploration
3.46
article

Is OSSO a Significant Contributor to the Unknown UV Absorber in Venus' Atmosphere?

Joanna Victoria Egan, D. R. Marsh, J. M. C. Plane, Alexander D. James, Franck Lefèvre, James Manners, Aurélien Stolzenbach, S. Lebonnois, Wuhu Feng
article en
3 citations

Abstract

Abstract It has been proposed that two isomers of the SO dimer ( cis ‐ and trans ‐OSSO) are candidates for the unknown UV absorber in Venus' atmosphere because they have a good spectral match with the absorber, despite the low concentrations predicted by 1D photochemical models. Here OSSO chemistry (production from SO and loss by photolysis, thermal decomposition, and reaction with O and Cl) has been included in the photochemistry scheme of a 3D planetary climate model (PCM‐Venus) along with sulfur injection due to meteoric ablation. 1D multiple scattering radiative transfer modeling is then used to predict the resulting top‐of‐the‐atmosphere reflectance produced by OSSO. The modeled OSSO concentrations are shown to be ∼3 orders of magnitude too low to explain the observed absorbance levels, and the predicted ratio of the OSSO isomers provides an unsatisfactory match to the spectral shape of the unknown absorber.

Geophysical Research LettersVol. 52(4)
Met Office (GB), Centre National de la Recherche Scientifique (FR), University of Leeds (GB), École Polytechnique (FR), University of Leicester (GB), Université de Versailles Saint-Quentin-en-Yvelines (FR), Université Paris Sciences et Lettres (FR), Université Paris-Saclay (FR), École Normale Supérieure - PSL (FR), Sorbonne Université (FR), Laboratoire de Météorologie Dynamique (FR), National Centre for Atmospheric Science (GB), Laboratoire atmosphères, milieux, observations spatiales (FR), Instituto de Astrofísica de Andalucía (ES)
Sight Research UK, Engineering and Physical Sciences Research Council, Natural Environment Research Council, Science and Technology Facilities Council
Climate action
Openalex Percentile: Top 9%
Planetary Science and Exploration
3.46
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