Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk
- Autores
- Brunini, Adrián
- Año de publicación
- 2002
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- In this paper we report numerical simulations of the dynamical evolution of the region a > 50 AU. We found that some dynamical effects such as high-order secular resonances with the rate of precession of Neptune's node of the form kΩ· − Ω·Nep with k = 4,5, ... or combined mean motion resonances with Uranus and Neptune of the form knN + jnU + mn ∼ 0 may increase the area of a very thin primordial disk in this region by a factor of up to 2 after 4.5 Gy of evolution.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata - Materia
-
Astronomía
Kuiper Belt
comets: general
solar system: general - 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:10915/123645
Ver los metadatos del registro completo
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Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin diskBrunini, AdriánAstronomíaKuiper Beltcomets: generalsolar system: generalIn this paper we report numerical simulations of the dynamical evolution of the region a > 50 AU. We found that some dynamical effects such as high-order secular resonances with the rate of precession of Neptune's node of the form kΩ· − Ω·<sub>Nep</sub> with k = 4,5, ... or combined mean motion resonances with Uranus and Neptune of the form kn<sub>N</sub> + jn<sub>U</sub> + mn ∼ 0 may increase the area of a very thin primordial disk in this region by a factor of up to 2 after 4.5 Gy of evolution.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2002-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf1129-1134http://sedici.unlp.edu.ar/handle/10915/123645enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/issn/1432-0746info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20021198info: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:UNLP2025-10-22T17:10:25Zoai:sedici.unlp.edu.ar:10915/123645Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:10:25.601SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk |
| title |
Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk |
| spellingShingle |
Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk Brunini, Adrián Astronomía Kuiper Belt comets: general solar system: general |
| title_short |
Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk |
| title_full |
Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk |
| title_fullStr |
Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk |
| title_full_unstemmed |
Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk |
| title_sort |
Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk |
| dc.creator.none.fl_str_mv |
Brunini, Adrián |
| author |
Brunini, Adrián |
| author_facet |
Brunini, Adrián |
| author_role |
author |
| dc.subject.none.fl_str_mv |
Astronomía Kuiper Belt comets: general solar system: general |
| topic |
Astronomía Kuiper Belt comets: general solar system: general |
| dc.description.none.fl_txt_mv |
In this paper we report numerical simulations of the dynamical evolution of the region a > 50 AU. We found that some dynamical effects such as high-order secular resonances with the rate of precession of Neptune's node of the form kΩ· − Ω·<sub>Nep</sub> with k = 4,5, ... or combined mean motion resonances with Uranus and Neptune of the form kn<sub>N</sub> + jn<sub>U</sub> + mn ∼ 0 may increase the area of a very thin primordial disk in this region by a factor of up to 2 after 4.5 Gy of evolution. Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata |
| description |
In this paper we report numerical simulations of the dynamical evolution of the region a > 50 AU. We found that some dynamical effects such as high-order secular resonances with the rate of precession of Neptune's node of the form kΩ· − Ω·<sub>Nep</sub> with k = 4,5, ... or combined mean motion resonances with Uranus and Neptune of the form kn<sub>N</sub> + jn<sub>U</sub> + mn ∼ 0 may increase the area of a very thin primordial disk in this region by a factor of up to 2 after 4.5 Gy of evolution. |
| publishDate |
2002 |
| dc.date.none.fl_str_mv |
2002-11 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/123645 |
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http://sedici.unlp.edu.ar/handle/10915/123645 |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/issn/0004-6361 info:eu-repo/semantics/altIdentifier/issn/1432-0746 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20021198 |
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openAccess |
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