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Updated: Jan 24, 2026

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Computation of Atmospheric Concentrations of Molecular Clusters from ab initio Thermochemistry
Published on: April 8, 2020
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Chlorine-sulfur oxides in the Venusian atmosphere: Benchmark data from computational spectroscopy
Luigi Crisci1, Tarek Trabelsi2, Joseph S Francisco3
1Scuola Superiore Meridionale, Largo San Marcellino 10, 80138 Napoli, Italy.
The Journal of Chemical Physics
|January 23, 2026
Summary
Researchers characterized chlorine-sulfur oxides (Cl2SOn) crucial for Venus
Area of Science:
- Planetary Science
- Atmospheric Chemistry
- Computational Chemistry
Background:
- Chlorine-sulfur oxides (Cl2SOn, n=1-4) are vital intermediates in Venus's atmospheric sulfur and chlorine cycles.
- These compounds influence the formation of sulfuric acid (H2SO4) clouds on Venus.
- Higher oxidation state Cl2SOn species are largely uncharacterized, lacking structural and spectroscopic data.
Purpose of the Study:
- To computationally determine the equilibrium geometries, rotational constants, and vibrational frequencies for the Cl2SOn series.
- To provide accurate spectroscopic parameters for uncharacterized higher oxidation state chlorine-sulfur oxides.
- To aid in the identification of these reactive species in laboratory and planetary observations.
Main Methods:
- Employed explicitly correlated ab initio methods for high-accuracy electronic structure calculations.
- Utilized second-order vibrational perturbation theory to account for anharmonic vibrational effects.
- Calculated equilibrium geometries, rotational constants, and anharmonic vibrational frequencies for Cl2SOn (n=1-4).
Main Results:
- Generated a consistent dataset of spectroscopic parameters for the Cl2SOn series.
- Achieved high accuracy by balancing electron correlation and anharmonic effects, closely matching existing experimental data.
- Extended predictive accuracy to higher, previously uncharacterized, chlorine-sulfur oxide species.
Conclusions:
- The study provides the first comprehensive reference data for Cl2SOn species.
- Predicted spectroscopic features will aid in identifying these intermediates in Venus's atmosphere.
- Findings will support the interpretation of data from upcoming Venus missions like EnVision and VERITAS.
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