Dynamical Behaviour of Asteroids in the Region a < 2 AU

Autores
Lopez Garcia, Francisco; Brunini, Adrián
Año de publicación
2001
Idioma
español castellano
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
We carried out a series of numerical simulations of the dynamical evolution of test particles and real asteroids in the inner region of the Solar System. We explored two different scenarios: i) including terrestrial planets plus Jupiter and Saturn and ii) including all the planets (except Pluto). We found that there are possible zones of orbital stability where planetesimals may survive 100 Myr. Secular resonances with the inner planets and mean motion commensurabilities with both the inner and outer planets play a key role in the dynamical evolution of this region.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Astronomía
Ciencias Exactas
dynamical evolution
asteroids
orbital stability
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/141381

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spelling Dynamical Behaviour of Asteroids in the Region a < 2 AULopez Garcia, FranciscoBrunini, AdriánAstronomíaCiencias Exactasdynamical evolutionasteroidsorbital stabilityWe carried out a series of numerical simulations of the dynamical evolution of test particles and real asteroids in the inner region of the Solar System. We explored two different scenarios: i) including terrestrial planets plus Jupiter and Saturn and ii) including all the planets (except Pluto). We found that there are possible zones of orbital stability where planetesimals may survive 100 Myr. Secular resonances with the inner planets and mean motion commensurabilities with both the inner and outer planets play a key role in the dynamical evolution of this region.Facultad de Ciencias Astronómicas y Geofísicas2001info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf417-422http://sedici.unlp.edu.ar/handle/10915/141381spainfo:eu-repo/semantics/altIdentifier/doi/10.1007/978-94-017-2304-6_33info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:13:01Zoai:sedici.unlp.edu.ar:10915/141381Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:13:01.427SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Dynamical Behaviour of Asteroids in the Region a < 2 AU
title Dynamical Behaviour of Asteroids in the Region a < 2 AU
spellingShingle Dynamical Behaviour of Asteroids in the Region a < 2 AU
Lopez Garcia, Francisco
Astronomía
Ciencias Exactas
dynamical evolution
asteroids
orbital stability
title_short Dynamical Behaviour of Asteroids in the Region a < 2 AU
title_full Dynamical Behaviour of Asteroids in the Region a < 2 AU
title_fullStr Dynamical Behaviour of Asteroids in the Region a < 2 AU
title_full_unstemmed Dynamical Behaviour of Asteroids in the Region a < 2 AU
title_sort Dynamical Behaviour of Asteroids in the Region a < 2 AU
dc.creator.none.fl_str_mv Lopez Garcia, Francisco
Brunini, Adrián
author Lopez Garcia, Francisco
author_facet Lopez Garcia, Francisco
Brunini, Adrián
author_role author
author2 Brunini, Adrián
author2_role author
dc.subject.none.fl_str_mv Astronomía
Ciencias Exactas
dynamical evolution
asteroids
orbital stability
topic Astronomía
Ciencias Exactas
dynamical evolution
asteroids
orbital stability
dc.description.none.fl_txt_mv We carried out a series of numerical simulations of the dynamical evolution of test particles and real asteroids in the inner region of the Solar System. We explored two different scenarios: i) including terrestrial planets plus Jupiter and Saturn and ii) including all the planets (except Pluto). We found that there are possible zones of orbital stability where planetesimals may survive 100 Myr. Secular resonances with the inner planets and mean motion commensurabilities with both the inner and outer planets play a key role in the dynamical evolution of this region.
Facultad de Ciencias Astronómicas y Geofísicas
description We carried out a series of numerical simulations of the dynamical evolution of test particles and real asteroids in the inner region of the Solar System. We explored two different scenarios: i) including terrestrial planets plus Jupiter and Saturn and ii) including all the planets (except Pluto). We found that there are possible zones of orbital stability where planetesimals may survive 100 Myr. Secular resonances with the inner planets and mean motion commensurabilities with both the inner and outer planets play a key role in the dynamical evolution of this region.
publishDate 2001
dc.date.none.fl_str_mv 2001
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http://purl.org/coar/resource_type/c_5794
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status_str publishedVersion
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url http://sedici.unlp.edu.ar/handle/10915/141381
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language spa
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1007/978-94-017-2304-6_33
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Creative Commons Attribution 4.0 International (CC BY 4.0)
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Creative Commons Attribution 4.0 International (CC BY 4.0)
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417-422
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