On the accretion of Uranus and Neptune

Autores
Brunini, Adrián; Melita, Mario Daniel
Año de publicación
2002
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In this paper, we discuss some problems concerning the formation of Uranus and Neptune. We find that the adoption of reduced Hill spheres as the region of close interaction between planetesimals introduces an enhancement of the gravitational cross-sections in previous numerical simulations. We also discuss a way to make possible the formation of Uranus and Neptune on time-scales shorter than the age of the Solar system.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
Accretion, accretion discs
Planets and satellites: formation
Planets and satellites: individual: Neptune
Planets and satellites: individual: Uranus
Solar system: formation
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/83168
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/83168
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling On the accretion of Uranus and NeptuneBrunini, AdriánMelita, Mario DanielCiencias AstronómicasAccretion, accretion discsPlanets and satellites: formationPlanets and satellites: individual: NeptunePlanets and satellites: individual: UranusSolar system: formationIn this paper, we discuss some problems concerning the formation of Uranus and Neptune. We find that the adoption of reduced Hill spheres as the region of close interaction between planetesimals introduces an enhancement of the gravitational cross-sections in previous numerical simulations. We also discuss a way to make possible the formation of Uranus and Neptune on time-scales shorter than the age of the Solar system.Facultad de Ciencias Astronómicas y Geofísicas2002info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf184-186http://sedici.unlp.edu.ar/handle/10915/83168enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1046/j.1365-8711.2002.05104.xinfo: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:UNLP2025-09-29T11:15:50Zoai:sedici.unlp.edu.ar:10915/83168Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:15:50.871SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv On the accretion of Uranus and Neptune
title On the accretion of Uranus and Neptune
spellingShingle On the accretion of Uranus and Neptune
Brunini, Adrián
Ciencias Astronómicas
Accretion, accretion discs
Planets and satellites: formation
Planets and satellites: individual: Neptune
Planets and satellites: individual: Uranus
Solar system: formation
title_short On the accretion of Uranus and Neptune
title_full On the accretion of Uranus and Neptune
title_fullStr On the accretion of Uranus and Neptune
title_full_unstemmed On the accretion of Uranus and Neptune
title_sort On the accretion of Uranus and Neptune
dc.creator.none.fl_str_mv Brunini, Adrián
Melita, Mario Daniel
author Brunini, Adrián
author_facet Brunini, Adrián
Melita, Mario Daniel
author_role author
author2 Melita, Mario Daniel
author2_role author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Accretion, accretion discs
Planets and satellites: formation
Planets and satellites: individual: Neptune
Planets and satellites: individual: Uranus
Solar system: formation
topic Ciencias Astronómicas
Accretion, accretion discs
Planets and satellites: formation
Planets and satellites: individual: Neptune
Planets and satellites: individual: Uranus
Solar system: formation
dc.description.none.fl_txt_mv In this paper, we discuss some problems concerning the formation of Uranus and Neptune. We find that the adoption of reduced Hill spheres as the region of close interaction between planetesimals introduces an enhancement of the gravitational cross-sections in previous numerical simulations. We also discuss a way to make possible the formation of Uranus and Neptune on time-scales shorter than the age of the Solar system.
Facultad de Ciencias Astronómicas y Geofísicas
description In this paper, we discuss some problems concerning the formation of Uranus and Neptune. We find that the adoption of reduced Hill spheres as the region of close interaction between planetesimals introduces an enhancement of the gravitational cross-sections in previous numerical simulations. We also discuss a way to make possible the formation of Uranus and Neptune on time-scales shorter than the age of the Solar system.
publishDate 2002
dc.date.none.fl_str_mv 2002
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/83168
url http://sedici.unlp.edu.ar/handle/10915/83168
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0035-8711
info:eu-repo/semantics/altIdentifier/doi/10.1046/j.1365-8711.2002.05104.x
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
184-186
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.070432

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