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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/202789
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T10:17:43Zoai: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:34982025-09-29 10:17:43.671CONICET 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 |
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1844614132565803008 |
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13.070432 |