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dc.contributor.authorRimmer, Paul .B.
dc.contributor.authorJordan, Sean
dc.contributor.authorConstantinou, Tereza
dc.contributor.authorWoitke, Peter
dc.contributor.authorShorttle, Oliver
dc.contributor.authorHobbs, Richard
dc.contributor.authorPaschodimas, Alessia
dc.date.accessioned2021-09-22T14:30:07Z
dc.date.available2021-09-22T14:30:07Z
dc.date.issued2021-08
dc.identifier.citationRimmer , P B , Jordan , S , Constantinou , T , Woitke , P , Shorttle , O , Hobbs , R & Paschodimas , A 2021 , ' Hydroxide salts in the clouds of Venus : their effect on the sulfur cycle and cloud droplet pH ' , The Planetary Science Journal , vol. 2 , no. 4 , 133 . https://doi.org/10.3847/PSJ/ac0156en
dc.identifier.issn2632-3338
dc.identifier.otherPURE: 275886131
dc.identifier.otherPURE UUID: 614cd2b2-4ec6-459e-8b15-2e47454561f9
dc.identifier.otherRIS: urn:E917FEA12EEBE1865A9AAA423E1098AA
dc.identifier.otherScopus: 85114504386
dc.identifier.urihttp://hdl.handle.net/10023/24002
dc.descriptionP.B.R. thanks the Simons Foundation for funding (SCOL awards 599634). P.W. acknowledges funding from the European Union H2020-MSCA-ITN-2019 under Grant Agreement no. 860470 (CHAMELEON).en
dc.description.abstractThe depletion of SO2 and H2O in and above the clouds of Venus (45-65 km) cannot be explained by known gasphase chemistry and the observed composition of the atmosphere. We apply a full-atmosphere model of Venus to investigate three potential explanations for the SO2 and H2O depletion: (1) varying the below-cloud water vapor (H2O), (2) varying the below-cloud sulfur dioxide (SO2), and (3) the incorporation of chemical reactions inside the sulfuric acid cloud droplets. We find that increasing the below-cloud H2O to explain the SO2 depletion results in a cloud top that is 20 km too high, above-cloud O2 three orders of magnitude greater than observational upper limits, and no SO above 80 km. The SO2 depletion can be explained by decreasing the below-cloud SO2 to 20 ppm. The depletion of SO2 in the clouds can also be explained by the SO2 dissolving into the clouds, if the droplets contain hydroxide salts. These salts buffer the cloud pH. The amount of salts sufficient to explain the SO2 depletion entails a droplet pH of ∼1 at 50 km. Because sulfuric acid is constantly condensing out into the cloud droplets, there must be a continuous and pervasive flux of salts of ≈10-13 mol cm-2 s-1 driving the cloud droplet chemistry. An atmospheric probe can test both of these explanations by measuring the pH of the cloud droplets and the concentrations of gas-phase SO2 below the clouds.
dc.format.extent25
dc.language.isoeng
dc.relation.ispartofThe Planetary Science Journalen
dc.rightsCopyright © 2021. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.en
dc.subjectCloudsen
dc.subjectPlanetary atmospheresen
dc.subjectVenusen
dc.subjectWater vaporen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleHydroxide salts in the clouds of Venus : their effect on the sulfur cycle and cloud droplet pHen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.St Andrews Centre for Exoplanet Scienceen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.3847/PSJ/ac0156
dc.description.statusPeer revieweden


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