Dynamical origin of V-type asteroids outside the Vesta family

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) cr...

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Autores principales: Roig, Fernando, Folonier, Hugo, Beaugé, Cristián, Ribeiro, Anderson O.
Formato: Objeto de conferencia
Lenguaje:Inglés
Publicado: 2011
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/167648
Aporte de:
id I19-R120-10915-167648
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spelling I19-R120-10915-1676482024-07-01T20:02:25Z http://sedici.unlp.edu.ar/handle/10915/167648 Dynamical origin of V-type asteroids outside the Vesta family Roig, Fernando Folonier, Hugo Beaugé, Cristián Ribeiro, Anderson O. 2011-07 2012 2024-07-01T16:55:13Z en Ciencias Astronómicas dynamical evolution Vesta family V-type asteroids 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 Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 307-317
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
dynamical evolution
Vesta family
V-type asteroids
spellingShingle Ciencias Astronómicas
dynamical evolution
Vesta family
V-type asteroids
Roig, Fernando
Folonier, Hugo
Beaugé, Cristián
Ribeiro, Anderson O.
Dynamical origin of V-type asteroids outside the Vesta family
topic_facet Ciencias Astronómicas
dynamical evolution
Vesta family
V-type asteroids
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.
format Objeto de conferencia
Objeto de conferencia
author Roig, Fernando
Folonier, Hugo
Beaugé, Cristián
Ribeiro, Anderson O.
author_facet Roig, Fernando
Folonier, Hugo
Beaugé, Cristián
Ribeiro, Anderson O.
author_sort Roig, Fernando
title Dynamical origin of V-type asteroids outside the Vesta family
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
publishDate 2011
url http://sedici.unlp.edu.ar/handle/10915/167648
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AT folonierhugo dynamicaloriginofvtypeasteroidsoutsidethevestafamily
AT beaugecristian dynamicaloriginofvtypeasteroidsoutsidethevestafamily
AT ribeiroandersono dynamicaloriginofvtypeasteroidsoutsidethevestafamily
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