Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk

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 combi...

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Autor principal: Brunini, Adrián
Formato: Articulo
Lenguaje:Inglés
Publicado: 2002
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/123645
Aporte de:SEDICI (UNLP) de Universidad Nacional de La Plata Ver origen
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spelling I19-R120-10915-1236452021-08-27T20:08:47Z http://sedici.unlp.edu.ar/handle/10915/123645 issn:0004-6361 issn:1432-0746 Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk Brunini, Adrián 2002-11 2021-08-27T16:13:18Z en Astronomía Kuiper Belt comets: general solar system: general 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 Articulo Articulo 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 1129-1134
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
Kuiper Belt
comets: general
solar system: general
spellingShingle Astronomía
Kuiper Belt
comets: general
solar system: general
Brunini, Adrián
Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk
topic_facet Astronomía
Kuiper Belt
comets: general
solar system: general
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.
format Articulo
Articulo
author Brunini, Adrián
author_facet Brunini, Adrián
author_sort Brunini, Adrián
title Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk
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
publishDate 2002
url http://sedici.unlp.edu.ar/handle/10915/123645
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