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  • Presentation | P31H: The Synergy Among Theoretical Methods, Laboratory Studies, and Atmospheric Modeling: Chemistry, Photochemistry, and Cloud Processes in Planetary Atmospheres I Poster
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  • P31H-2628: INSIGHTS INTO CATALYTIC CHLORINE OXIDATION OF CO IN THE VENUS MESOSPHERE
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  • Board 2628‚ Hall EFG (Poster Hall)
    NOLA CC
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Author(s):
Frank Winiberg, NASA Jet Propulsion Laboratory, California Institute of Technology (First Author)
Wen Chao, NASA Jet Propulsion Laboratory, California Institute of Technology (Presenting Author)
Mads Sulbaek Andersen, California State University Northridge
Gregory Jones, University of Florida
Robert Skog, University of Helsinki
Benjamin Frandsen, University of Helsinki
Charles Markus, University of Texas, San Antonio
Franklin Mills, Australian National University
Yuk Yung, California Institute of Technology
Carl Percival, NASA Jet Propulsion Laboratory
Mitchio Okumura, California Institute of Technology


Telescopes and satellites have extensively looked at Earth's evil twin, Venus, but they have yet to observe oxygen - this goes in the face of computer simulations of the atmosphere that predict it must be there at levels high enough to detect. In the laboratory we have studied particular chemical reactions, under conditions relevant to Venus' upper atmosphere, that may hold the key to understanding why there is no observed molecular oxygen on Venus. In particular, we have investigated whether reactions between chlorine and carbon monoxide might be converting oxygen to carbon dioxide. We will show our equipment, results from our experiments, and updated computer simulations of Venus' atmosphere with our new laboratory results.



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