Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons

Autores
Sucerquia, Mario; Alvarado Montes, Jaime A.; Bayo, Amelia; Cuadra, Jorge; Cuello, Juan Nicolás; Giuppone, Cristian Andrés; Montesinos, Matías; Olofsson, J.; Schwab, Christian; Spitler, Lee; Zuluaga, Jorge I
Año de publicación
2022
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In recent years, technical and theoretical work to detect moons and rings around exoplanets has been attempted. The small mass/size ratios between moons and planets means this is very challenging, having only one exoplanetary system where spotting an exomoon might be feasible (i.e. Kepler-1625b i). In this work, we study the dynamical evolution of ringed exomoons, dubbed cronomoons after their similarity with Cronus (Greek for Saturn), and after Chronos (the epitome of time), following the Transit Timing Variations and Transit Duration Variation that they produce on their host planet. Cronomoons have extended systems of rings that make them appear bigger than they actually are when transiting in front of their host star. We explore different possible scenarios that could lead to the formation of such circumsatellital rings, and through the study of the dynamical/thermodynamic stability and lifespan of their dust and ice ring particles, we found that an isolated cronomoon can survive for time-scales long enough to be detected and followed up. If these objects exist, cronomoons' rings will exhibit gaps similar to Saturn's Cassini Division and analogous to the asteroid belt's Kirkwood gaps but instead raised due to resonances induced by the host planet. Finally, we analyse the case of Kepler-1625b i under the scope of this work, finding that the controversial giant moon could instead be an Earth-mass cronomoon. From a theoretical perspective, this scenario can contribute to a better interpretation of the underlying phenomenology in current and future observations.
Fil: Sucerquia, Mario. Universidad de Valparaíso; Chile
Fil: Alvarado Montes, Jaime A.. Macquarie University; Australia
Fil: Bayo, Amelia. Universidad de Valparaíso; Chile
Fil: Cuadra, Jorge. Universidad de Valparaíso; Chile. Universidad Adolfo Ibañez; Chile
Fil: Cuello, Juan Nicolás. Universite Grenoble Alpes.; Francia. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Giuppone, Cristian Andrés. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Montesinos, Matías. Universidad de Valparaíso; Chile. Universidad de Viña del Mar (uvm); Chile
Fil: Olofsson, J.. Universidad de Valparaíso; Chile
Fil: Schwab, Christian. Macquarie University; Australia
Fil: Spitler, Lee. Macquarie University; Australia
Fil: Zuluaga, Jorge I. Universidad de Antioquia; Colombia
Materia
METHODS: ANALYTICAL
PLANETS AND SATELLITES: DETECTION
PLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITY
PLANETS AND SATELLITES: RINGS
TECHNIQUES: PHOTOMETRIC
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/202789
Acceder
id CONICETDig_0ff570dbc6485c37ef9b72f281d67e7d
oai_identifier_str oai:ri.conicet.gov.ar:11336/202789
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Cronomoons: Origin, dynamics, and light-curve features of ringed exomoonsSucerquia, MarioAlvarado Montes, Jaime A.Bayo, AmeliaCuadra, JorgeCuello, Juan NicolásGiuppone, Cristian AndrésMontesinos, MatíasOlofsson, J.Schwab, ChristianSpitler, LeeZuluaga, Jorge IMETHODS: ANALYTICALPLANETS AND SATELLITES: DETECTIONPLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITYPLANETS AND SATELLITES: RINGSTECHNIQUES: PHOTOMETRIChttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In recent years, technical and theoretical work to detect moons and rings around exoplanets has been attempted. The small mass/size ratios between moons and planets means this is very challenging, having only one exoplanetary system where spotting an exomoon might be feasible (i.e. Kepler-1625b i). In this work, we study the dynamical evolution of ringed exomoons, dubbed cronomoons after their similarity with Cronus (Greek for Saturn), and after Chronos (the epitome of time), following the Transit Timing Variations and Transit Duration Variation that they produce on their host planet. Cronomoons have extended systems of rings that make them appear bigger than they actually are when transiting in front of their host star. We explore different possible scenarios that could lead to the formation of such circumsatellital rings, and through the study of the dynamical/thermodynamic stability and lifespan of their dust and ice ring particles, we found that an isolated cronomoon can survive for time-scales long enough to be detected and followed up. If these objects exist, cronomoons' rings will exhibit gaps similar to Saturn's Cassini Division and analogous to the asteroid belt's Kirkwood gaps but instead raised due to resonances induced by the host planet. Finally, we analyse the case of Kepler-1625b i under the scope of this work, finding that the controversial giant moon could instead be an Earth-mass cronomoon. From a theoretical perspective, this scenario can contribute to a better interpretation of the underlying phenomenology in current and future observations.Fil: Sucerquia, Mario. Universidad de Valparaíso; ChileFil: Alvarado Montes, Jaime A.. Macquarie University; AustraliaFil: Bayo, Amelia. Universidad de Valparaíso; ChileFil: Cuadra, Jorge. Universidad de Valparaíso; Chile. Universidad Adolfo Ibañez; ChileFil: Cuello, Juan Nicolás. Universite Grenoble Alpes.; Francia. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Giuppone, Cristian Andrés. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaFil: Montesinos, Matías. Universidad de Valparaíso; Chile. Universidad de Viña del Mar (uvm); ChileFil: Olofsson, J.. Universidad de Valparaíso; ChileFil: Schwab, Christian. Macquarie University; AustraliaFil: Spitler, Lee. Macquarie University; AustraliaFil: Zuluaga, Jorge I. Universidad de Antioquia; ColombiaOxford Univ Press Inc2022-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/202789Sucerquia, Mario; Alvarado Montes, Jaime A.; Bayo, Amelia; Cuadra, Jorge; Cuello, Juan Nicolás; et al.; Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons; Oxford Univ Press Inc; Monthly Notices of the Royal Astronomical Society; 512; 1; 5-2022; 1032-10440035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stab3531info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/512/1/1032/6461099?redirectedFrom=fulltextinfo:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2112.02687info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:48:01Zoai:ri.conicet.gov.ar:11336/202789instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:48:01.537CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons
title Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons
spellingShingle Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons
Sucerquia, Mario
METHODS: ANALYTICAL
PLANETS AND SATELLITES: DETECTION
PLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITY
PLANETS AND SATELLITES: RINGS
TECHNIQUES: PHOTOMETRIC
title_short Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons
title_full Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons
title_fullStr Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons
title_full_unstemmed Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons
title_sort Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons
dc.creator.none.fl_str_mv Sucerquia, Mario
Alvarado Montes, Jaime A.
Bayo, Amelia
Cuadra, Jorge
Cuello, Juan Nicolás
Giuppone, Cristian Andrés
Montesinos, Matías
Olofsson, J.
Schwab, Christian
Spitler, Lee
Zuluaga, Jorge I
author Sucerquia, Mario
author_facet Sucerquia, Mario
Alvarado Montes, Jaime A.
Bayo, Amelia
Cuadra, Jorge
Cuello, Juan Nicolás
Giuppone, Cristian Andrés
Montesinos, Matías
Olofsson, J.
Schwab, Christian
Spitler, Lee
Zuluaga, Jorge I
author_role author
author2 Alvarado Montes, Jaime A.
Bayo, Amelia
Cuadra, Jorge
Cuello, Juan Nicolás
Giuppone, Cristian Andrés
Montesinos, Matías
Olofsson, J.
Schwab, Christian
Spitler, Lee
Zuluaga, Jorge I
author2_role author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv METHODS: ANALYTICAL
PLANETS AND SATELLITES: DETECTION
PLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITY
PLANETS AND SATELLITES: RINGS
TECHNIQUES: PHOTOMETRIC
topic METHODS: ANALYTICAL
PLANETS AND SATELLITES: DETECTION
PLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITY
PLANETS AND SATELLITES: RINGS
TECHNIQUES: PHOTOMETRIC
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In recent years, technical and theoretical work to detect moons and rings around exoplanets has been attempted. The small mass/size ratios between moons and planets means this is very challenging, having only one exoplanetary system where spotting an exomoon might be feasible (i.e. Kepler-1625b i). In this work, we study the dynamical evolution of ringed exomoons, dubbed cronomoons after their similarity with Cronus (Greek for Saturn), and after Chronos (the epitome of time), following the Transit Timing Variations and Transit Duration Variation that they produce on their host planet. Cronomoons have extended systems of rings that make them appear bigger than they actually are when transiting in front of their host star. We explore different possible scenarios that could lead to the formation of such circumsatellital rings, and through the study of the dynamical/thermodynamic stability and lifespan of their dust and ice ring particles, we found that an isolated cronomoon can survive for time-scales long enough to be detected and followed up. If these objects exist, cronomoons' rings will exhibit gaps similar to Saturn's Cassini Division and analogous to the asteroid belt's Kirkwood gaps but instead raised due to resonances induced by the host planet. Finally, we analyse the case of Kepler-1625b i under the scope of this work, finding that the controversial giant moon could instead be an Earth-mass cronomoon. From a theoretical perspective, this scenario can contribute to a better interpretation of the underlying phenomenology in current and future observations.
Fil: Sucerquia, Mario. Universidad de Valparaíso; Chile
Fil: Alvarado Montes, Jaime A.. Macquarie University; Australia
Fil: Bayo, Amelia. Universidad de Valparaíso; Chile
Fil: Cuadra, Jorge. Universidad de Valparaíso; Chile. Universidad Adolfo Ibañez; Chile
Fil: Cuello, Juan Nicolás. Universite Grenoble Alpes.; Francia. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Giuppone, Cristian Andrés. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Montesinos, Matías. Universidad de Valparaíso; Chile. Universidad de Viña del Mar (uvm); Chile
Fil: Olofsson, J.. Universidad de Valparaíso; Chile
Fil: Schwab, Christian. Macquarie University; Australia
Fil: Spitler, Lee. Macquarie University; Australia
Fil: Zuluaga, Jorge I. Universidad de Antioquia; Colombia
description In recent years, technical and theoretical work to detect moons and rings around exoplanets has been attempted. The small mass/size ratios between moons and planets means this is very challenging, having only one exoplanetary system where spotting an exomoon might be feasible (i.e. Kepler-1625b i). In this work, we study the dynamical evolution of ringed exomoons, dubbed cronomoons after their similarity with Cronus (Greek for Saturn), and after Chronos (the epitome of time), following the Transit Timing Variations and Transit Duration Variation that they produce on their host planet. Cronomoons have extended systems of rings that make them appear bigger than they actually are when transiting in front of their host star. We explore different possible scenarios that could lead to the formation of such circumsatellital rings, and through the study of the dynamical/thermodynamic stability and lifespan of their dust and ice ring particles, we found that an isolated cronomoon can survive for time-scales long enough to be detected and followed up. If these objects exist, cronomoons' rings will exhibit gaps similar to Saturn's Cassini Division and analogous to the asteroid belt's Kirkwood gaps but instead raised due to resonances induced by the host planet. Finally, we analyse the case of Kepler-1625b i under the scope of this work, finding that the controversial giant moon could instead be an Earth-mass cronomoon. From a theoretical perspective, this scenario can contribute to a better interpretation of the underlying phenomenology in current and future observations.
publishDate 2022
dc.date.none.fl_str_mv 2022-05
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/202789
Sucerquia, Mario; Alvarado Montes, Jaime A.; Bayo, Amelia; Cuadra, Jorge; Cuello, Juan Nicolás; et al.; Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons; Oxford Univ Press Inc; Monthly Notices of the Royal Astronomical Society; 512; 1; 5-2022; 1032-1044
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/202789
identifier_str_mv Sucerquia, Mario; Alvarado Montes, Jaime A.; Bayo, Amelia; Cuadra, Jorge; Cuello, Juan Nicolás; et al.; Cronomoons: Origin, dynamics, and light-curve features of ringed exomoons; Oxford Univ Press Inc; Monthly Notices of the Royal Astronomical Society; 512; 1; 5-2022; 1032-1044
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stab3531
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/512/1/1032/6461099?redirectedFrom=fulltext
info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2112.02687
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Oxford Univ Press Inc
publisher.none.fl_str_mv Oxford Univ Press Inc
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1846782185687744512
score 13.229304

Publicaciones similares