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
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/141381
Ver los metadatos del registro completo
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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 |
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2001 |
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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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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
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openAccess |
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