Dynamical origin of V-type asteroids outside the Vesta family
- Autores
- Roig, Fernando; Folonier, Hugo; Beaugé, Cristián; Ribeiro, Anderson O.
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- We review some recent results on the long term dynamical evolution of V-type asteroids that point to their origin as fugitives from the Vesta family. Three scenarios are explored: (i) interplay of weak mean motion and non linear secular resonances in the inner Belt with the Yarkovsky effect, (ii) crossing of the 3:1 mean motion resonance with Jupiter, and (iii) evolution by planetary encounters and resonance stickiness. These mechanisms may explain a large fraction of the V-type asteroids that are observed outside the Vesta family, but there are some particular cases that would need other explanations.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
dynamical evolution
Vesta family
V-type asteroids - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/167648
Ver los metadatos del registro completo
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Dynamical origin of V-type asteroids outside the Vesta familyRoig, FernandoFolonier, HugoBeaugé, CristiánRibeiro, Anderson O.Ciencias Astronómicasdynamical evolutionVesta familyV-type asteroidsWe review some recent results on the long term dynamical evolution of V-type asteroids that point to their origin as fugitives from the Vesta family. Three scenarios are explored: (i) interplay of weak mean motion and non linear secular resonances in the inner Belt with the Yarkovsky effect, (ii) crossing of the 3:1 mean motion resonance with Jupiter, and (iii) evolution by planetary encounters and resonance stickiness. These mechanisms may explain a large fraction of the V-type asteroids that are observed outside the Vesta family, but there are some particular cases that would need other explanations.Facultad de Ciencias Astronómicas y Geofísicas2011-07info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf307-317http://sedici.unlp.edu.ar/handle/10915/167648enginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:44:40Zoai:sedici.unlp.edu.ar:10915/167648Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:44:40.818SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Dynamical origin of V-type asteroids outside the Vesta family |
| title |
Dynamical origin of V-type asteroids outside the Vesta family |
| spellingShingle |
Dynamical origin of V-type asteroids outside the Vesta family Roig, Fernando Ciencias Astronómicas dynamical evolution Vesta family V-type asteroids |
| title_short |
Dynamical origin of V-type asteroids outside the Vesta family |
| title_full |
Dynamical origin of V-type asteroids outside the Vesta family |
| title_fullStr |
Dynamical origin of V-type asteroids outside the Vesta family |
| title_full_unstemmed |
Dynamical origin of V-type asteroids outside the Vesta family |
| title_sort |
Dynamical origin of V-type asteroids outside the Vesta family |
| dc.creator.none.fl_str_mv |
Roig, Fernando Folonier, Hugo Beaugé, Cristián Ribeiro, Anderson O. |
| author |
Roig, Fernando |
| author_facet |
Roig, Fernando Folonier, Hugo Beaugé, Cristián Ribeiro, Anderson O. |
| author_role |
author |
| author2 |
Folonier, Hugo Beaugé, Cristián Ribeiro, Anderson O. |
| author2_role |
author author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas dynamical evolution Vesta family V-type asteroids |
| topic |
Ciencias Astronómicas dynamical evolution Vesta family V-type asteroids |
| dc.description.none.fl_txt_mv |
We review some recent results on the long term dynamical evolution of V-type asteroids that point to their origin as fugitives from the Vesta family. Three scenarios are explored: (i) interplay of weak mean motion and non linear secular resonances in the inner Belt with the Yarkovsky effect, (ii) crossing of the 3:1 mean motion resonance with Jupiter, and (iii) evolution by planetary encounters and resonance stickiness. These mechanisms may explain a large fraction of the V-type asteroids that are observed outside the Vesta family, but there are some particular cases that would need other explanations. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
We review some recent results on the long term dynamical evolution of V-type asteroids that point to their origin as fugitives from the Vesta family. Three scenarios are explored: (i) interplay of weak mean motion and non linear secular resonances in the inner Belt with the Yarkovsky effect, (ii) crossing of the 3:1 mean motion resonance with Jupiter, and (iii) evolution by planetary encounters and resonance stickiness. These mechanisms may explain a large fraction of the V-type asteroids that are observed outside the Vesta family, but there are some particular cases that would need other explanations. |
| publishDate |
2011 |
| dc.date.none.fl_str_mv |
2011-07 |
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info:eu-repo/semantics/conferenceObject info:eu-repo/semantics/publishedVersion Objeto de conferencia http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
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conferenceObject |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/167648 |
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http://sedici.unlp.edu.ar/handle/10915/167648 |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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