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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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 |
work_keys_str_mv |
AT roigfernando dynamicaloriginofvtypeasteroidsoutsidethevestafamily AT folonierhugo dynamicaloriginofvtypeasteroidsoutsidethevestafamily AT beaugecristian dynamicaloriginofvtypeasteroidsoutsidethevestafamily AT ribeiroandersono dynamicaloriginofvtypeasteroidsoutsidethevestafamily |
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1807223540249788416 |