The origin of Jupiter's Great Red Spot

Jupiter's Great Red Spot (GRS) is the largest and longest-lived known vortex of all solar system planets but its lifetime is debated and its formation mechanism remains hidden. G. D. Cassini discovered in 1665 the presence of a dark oval at the GRS latitude, known as the “Permanent Spot” (PS) t...

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Autores: Sanchez Lavega, Agustin, García Melendo, Enrique José|||0000-0002-3354-1140, Legarreta, Jon J., Miró Jané, Arnau|||0000-0002-2772-6050, Soria Guerrero, Manel|||0000-0002-4112-6078, Ahrens Velásquez, Kevin
Formato: artículo
Fecha de publicación:2024
País:España
Recursos:Universitat Politècnica de Catalunya (UPC)
Repositorio:UPCommons. Portal del coneixement obert de la UPC
Idioma:inglés
OAI Identifier:oai:upcommons.upc.edu:2117/410483
Acesso em linha:https://hdl.handle.net/2117/410483
https://dx.doi.org/10.1029/2024GL108993
Access Level:acceso abierto
Palavra-chave:Jupiter (Planet)
Eddies
Vortex-motion
Júpiter (Planeta)
Remolins (Mecànica de fluids)
Vorticitat
Àrees temàtiques de la UPC::Física
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spelling The origin of Jupiter's Great Red SpotSanchez Lavega, AgustinGarcía Melendo, Enrique José|||0000-0002-3354-1140Legarreta, Jon J.Miró Jané, Arnau|||0000-0002-2772-6050Soria Guerrero, Manel|||0000-0002-4112-6078Ahrens Velásquez, KevinJupiter (Planet)EddiesVortex-motionJúpiter (Planeta)Remolins (Mecànica de fluids)VorticitatÀrees temàtiques de la UPC::FísicaJupiter's Great Red Spot (GRS) is the largest and longest-lived known vortex of all solar system planets but its lifetime is debated and its formation mechanism remains hidden. G. D. Cassini discovered in 1665 the presence of a dark oval at the GRS latitude, known as the “Permanent Spot” (PS) that was observed until 1713. We show from historical observations of its size evolution and motions that PS is unlikely to correspond to the current GRS, that was first observed in 1831. Numerical simulations rule out that the GRS formed by the merging of vortices or by a superstorm, but most likely formed from a flow disturbance between the two opposed Jovian zonal jets north and south of it. If so, the early GRS should have had a low tangential velocity so that its rotation velocity has increased over time as it has shrunk.ASL and JL were supported by Grupos Gobierno Vasco IT1742‐22 and by Grant PID2019‐109467GB‐I00 funded by MCIN/AEI/10.13039/501100011033/. EGM, AM, MS and KAV thankfully acknowledge the computer resources provided by Red Española de Supercomputación (RES) under the projects AECT‐2020‐1‐0005 and RESAECT‐2021‐2‐0009. We also acknowledge the Barcelona Supercomputing Center for awarding us access to the MareNostrum IV machine based in Barcelona, Spain and the Centro de Astrofísica de La Palma (IAC) for awarding us access to the La Palma machine based in La Palma, Spain. We acknowledge Josep María Gómez Forrellad for assisting in retrieving data from historical sources.20242024-06-2820242024-06-25journal articlehttp://purl.org/coar/resource_type/c_6501VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/2117/410483https://dx.doi.org/10.1029/2024GL108993reponame:UPCommons. Portal del coneixement obert de la UPCinstname:Universitat Politècnica de Catalunya (UPC)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2Attribution-NonCommercial-NoDerivatives 4.0 Internationalhttp://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessoai:upcommons.upc.edu:2117/4104832026-05-27T15:37:01Z
dc.title.none.fl_str_mv The origin of Jupiter's Great Red Spot
title The origin of Jupiter's Great Red Spot
spellingShingle The origin of Jupiter's Great Red Spot
Sanchez Lavega, Agustin
Jupiter (Planet)
Eddies
Vortex-motion
Júpiter (Planeta)
Remolins (Mecànica de fluids)
Vorticitat
Àrees temàtiques de la UPC::Física
title_short The origin of Jupiter's Great Red Spot
title_full The origin of Jupiter's Great Red Spot
title_fullStr The origin of Jupiter's Great Red Spot
title_full_unstemmed The origin of Jupiter's Great Red Spot
title_sort The origin of Jupiter's Great Red Spot
dc.creator.none.fl_str_mv Sanchez Lavega, Agustin
García Melendo, Enrique José|||0000-0002-3354-1140
Legarreta, Jon J.
Miró Jané, Arnau|||0000-0002-2772-6050
Soria Guerrero, Manel|||0000-0002-4112-6078
Ahrens Velásquez, Kevin
author Sanchez Lavega, Agustin
author_facet Sanchez Lavega, Agustin
García Melendo, Enrique José|||0000-0002-3354-1140
Legarreta, Jon J.
Miró Jané, Arnau|||0000-0002-2772-6050
Soria Guerrero, Manel|||0000-0002-4112-6078
Ahrens Velásquez, Kevin
author_role author
author2 García Melendo, Enrique José|||0000-0002-3354-1140
Legarreta, Jon J.
Miró Jané, Arnau|||0000-0002-2772-6050
Soria Guerrero, Manel|||0000-0002-4112-6078
Ahrens Velásquez, Kevin
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv Jupiter (Planet)
Eddies
Vortex-motion
Júpiter (Planeta)
Remolins (Mecànica de fluids)
Vorticitat
Àrees temàtiques de la UPC::Física
topic Jupiter (Planet)
Eddies
Vortex-motion
Júpiter (Planeta)
Remolins (Mecànica de fluids)
Vorticitat
Àrees temàtiques de la UPC::Física
description Jupiter's Great Red Spot (GRS) is the largest and longest-lived known vortex of all solar system planets but its lifetime is debated and its formation mechanism remains hidden. G. D. Cassini discovered in 1665 the presence of a dark oval at the GRS latitude, known as the “Permanent Spot” (PS) that was observed until 1713. We show from historical observations of its size evolution and motions that PS is unlikely to correspond to the current GRS, that was first observed in 1831. Numerical simulations rule out that the GRS formed by the merging of vortices or by a superstorm, but most likely formed from a flow disturbance between the two opposed Jovian zonal jets north and south of it. If so, the early GRS should have had a low tangential velocity so that its rotation velocity has increased over time as it has shrunk.
publishDate 2024
dc.date.none.fl_str_mv 2024
2024-06-28
2024
2024-06-25
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
VoR
http://purl.org/coar/version/c_970fb48d4fbd8a85
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/2117/410483
https://dx.doi.org/10.1029/2024GL108993
url https://hdl.handle.net/2117/410483
https://dx.doi.org/10.1029/2024GL108993
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution-NonCommercial-NoDerivatives 4.0 International
http://creativecommons.org/licenses/by-nc-nd/4.0/
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution-NonCommercial-NoDerivatives 4.0 International
http://creativecommons.org/licenses/by-nc-nd/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:UPCommons. Portal del coneixement obert de la UPC
instname:Universitat Politècnica de Catalunya (UPC)
instname_str Universitat Politècnica de Catalunya (UPC)
reponame_str UPCommons. Portal del coneixement obert de la UPC
collection UPCommons. Portal del coneixement obert de la UPC
repository.name.fl_str_mv
repository.mail.fl_str_mv
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