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...
| Autores: | , , , , , |
|---|---|
| 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 |
| id |
ES_2ce6b5eb95a1fa8e0b97dd17fa6979dc |
|---|---|
| oai_identifier_str |
oai:upcommons.upc.edu:2117/410483 |
| network_acronym_str |
ES |
| network_name_str |
España |
| repository_id_str |
|
| 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 |
|
| _version_ |
1869405273565691904 |
| score |
15,81155 |