Stratospheric aerosols and C6H6 in Jupiter's south polar region from JWST/MIRI observations
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited
| Autores: | , , , , , , , , , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/372809 |
| Acceso en línea: | http://hdl.handle.net/10261/372809 |
| Access Level: | acceso abierto |
| Palabra clave: | Planets and satellites: atmospheres Planets and satellites: aurorae Planets and satellites: composition Planets and satellites: gaseous planets |
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Stratospheric aerosols and C6H6 in Jupiter's south polar region from JWST/MIRI observations |
| title |
Stratospheric aerosols and C6H6 in Jupiter's south polar region from JWST/MIRI observations |
| spellingShingle |
Stratospheric aerosols and C6H6 in Jupiter's south polar region from JWST/MIRI observations Rodríguez-Ovalle, Pablo Planets and satellites: atmospheres Planets and satellites: aurorae Planets and satellites: composition Planets and satellites: gaseous planets |
| title_short |
Stratospheric aerosols and C6H6 in Jupiter's south polar region from JWST/MIRI observations |
| title_full |
Stratospheric aerosols and C6H6 in Jupiter's south polar region from JWST/MIRI observations |
| title_fullStr |
Stratospheric aerosols and C6H6 in Jupiter's south polar region from JWST/MIRI observations |
| title_full_unstemmed |
Stratospheric aerosols and C6H6 in Jupiter's south polar region from JWST/MIRI observations |
| title_sort |
Stratospheric aerosols and C6H6 in Jupiter's south polar region from JWST/MIRI observations |
| dc.creator.none.fl_str_mv |
Rodríguez-Ovalle, Pablo Guerlet, Sandrine Fouchet, T. Harkett, Jake Cavalié, Thibault Hue, Vincent Vinatier, S. López-Puertas, Manuel Fletcher, L. N. Lellouch, E. Hueso, Ricardo de Pater, Imke Orton, Glenn S. Roman, Michael T. Hammel, Heidi B. Milam, Stefanie N. King, Oliver R. T. |
| author |
Rodríguez-Ovalle, Pablo |
| author_facet |
Rodríguez-Ovalle, Pablo Guerlet, Sandrine Fouchet, T. Harkett, Jake Cavalié, Thibault Hue, Vincent Vinatier, S. López-Puertas, Manuel Fletcher, L. N. Lellouch, E. Hueso, Ricardo de Pater, Imke Orton, Glenn S. Roman, Michael T. Hammel, Heidi B. Milam, Stefanie N. King, Oliver R. T. |
| author_role |
author |
| author2 |
Guerlet, Sandrine Fouchet, T. Harkett, Jake Cavalié, Thibault Hue, Vincent Vinatier, S. López-Puertas, Manuel Fletcher, L. N. Lellouch, E. Hueso, Ricardo de Pater, Imke Orton, Glenn S. Roman, Michael T. Hammel, Heidi B. Milam, Stefanie N. King, Oliver R. T. |
| author2_role |
author author author author author author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
Université Paris Cité Gouvernement de la République française Agencia Estatal de Investigación (España) Science and Technology Facilities Council (UK) NASA Ministerio de Ciencia e Innovación (España) Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Planets and satellites: atmospheres Planets and satellites: aurorae Planets and satellites: composition Planets and satellites: gaseous planets |
| topic |
Planets and satellites: atmospheres Planets and satellites: aurorae Planets and satellites: composition Planets and satellites: gaseous planets |
| description |
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited |
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2024 |
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2024 2024 2024 |
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info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
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article |
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http://hdl.handle.net/10261/372809 |
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http://hdl.handle.net/10261/372809 |
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Inglés |
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Inglés |
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European Southern Observatory |
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European Southern Observatory |
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Stratospheric aerosols and C6H6 in Jupiter's south polar region from JWST/MIRI observationsRodríguez-Ovalle, PabloGuerlet, SandrineFouchet, T.Harkett, JakeCavalié, ThibaultHue, VincentVinatier, S.López-Puertas, ManuelFletcher, L. N.Lellouch, E.Hueso, Ricardode Pater, ImkeOrton, Glenn S.Roman, Michael T.Hammel, Heidi B.Milam, Stefanie N.King, Oliver R. T.Planets and satellites: atmospheresPlanets and satellites: auroraePlanets and satellites: compositionPlanets and satellites: gaseous planetsOpen Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly citedContext. The polar atmosphere of Jupiter is significantly affected by auroral activity, which can induce both thermal and chemical differences compared to the rest of the atmosphere. In particular, auroral activity enhances the production of various hydrocarbons, including benzene. Benzene could be a potential precursor to the formation of the stratospheric hazes. Aims. We investigated the spatial distribution of the benzene abundance across latitudes ranging from 50°S to 81°S and 17°S to 25°S. Additionally, we examined the chemical origin of polar aerosols and their latitudinal distribution. Methods. We employed James Webb Space Telescope (JWST) Mid InfraRed Instrument (MIRI) observations to measure the benzene abundance based on its emission at 674 cm‑1. Additionally, we examined the spectral dependence of the aerosol opacity within the 680–760 and 1380–1500 cm‑1 spectral ranges, and mapped their distribution from 80°S–50°S. Results. At latitudes lower than 60°S, benzene is found to be up to ten times more abundant compared to lower latitudes. This enhancement of C6H6 is well mixed longitudinally and not particularly concentrated inside the auroral oval. Photochemical models predict a decrease in the abundance as we approach the mid latitudes, but fail at polar latitudes as they do not include ion-neutral chemistry. Moreover, we find that the southern polar atmosphere is enriched with aerosols at ~10 mbar. The optical depth of the aerosols increases at latitudes poleward of ~60°S, similar to the enhancement of C6H6. These aerosols have spectral features similar to the aerosols of Titan and Saturn, and the mass loading is of ~1.2 ± 0.2 × 10‑4 g cm‑2. Finally, we quantified the impact of these aerosols on the retrieved temperature structure, causing a decrease in the temperature at pressure levels deeper than 10 mbar. Conclusions. We find that the auroral precipitation produces abundant stratospheric aerosols, which must play an important role in the chemistry and dynamics of the planet. © The Authors 2024This work is based on observations obtained with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program #1373 (Observations 2, 4 and 26), which is led by co-PIs Imke de Pater and Thierry Fouchet. Data from JWST programs 1246 and 1247 were used for wavelength calibration. P.R.O. was supported by an Université Paris-Cité contract. T.C. acknowledges funding from CNES and from the Programme National de Planétologie. V.H. acknowledges support from the French government under the France 2030 investment plan, as part of the Initiative d’Excellence d’Aix-Marseille Université – A*MIDEX AMX-22-CPJ-04. M.L.P. acknowledges financial support from the Agencia Estatal de Investigación, MCIN/AEI/ 10.13039/ 501100011033, through grants PID2022-141216NB-I00 and CEX2021- 001131-S. I.d.P. is in part supported by the Space Telescope Science Institute grant JWST-ERS-01373. L.N.F., M.T.R. and O.T.R.K. were supported by STFC Consolidated Grant reference ST/W00089X/1. J.H. was supported by an STFC studentship. H.B.H. and S.N.M. acknowledge support from NASA JWST Interdisciplinary Scientist grant 21-SMDSS21-0013. R.H. was supported by grant PID 2019-109467GB-I00 funded by MCIN/AEI/ 10.13039/501100011033/ and was also supported by Grupos Gobierno Vasco IT1742-22. For the purpose of open access, the author has applied a Creative Commons Attribution (CC BY) licence to the Author Accepted Manuscript version arising from this submission. Some of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004).Peer reviewedEuropean Southern ObservatoryUniversité Paris CitéGouvernement de la République françaiseAgencia Estatal de Investigación (España)Science and Technology Facilities Council (UK)NASAMinisterio de Ciencia e Innovación (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202420242024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/372809reponame:DIGITAL.CSIC. 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15.811543 |