Origin of slow-rotating minor bodies by tidal decoupling of binary pairs

Autores
Brunini, Adrian
Año de publicación
2017
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In this paper, we show that the decoupling of binary pairs by tidal interaction and Kozai oscillations acting together can generate single objects in a slow-rotation-rate state. This mechanism has the merit of not being strongly dependent on the size or shape of the objects. The key parameter leading the process is ω/n, the ratio between the rotation rate and the orbital mean motion of the binary, which must be > 1. The proposed mechanism could also operate in other populations of minor bodies.
Fil: Brunini, Adrian. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de la Patagonia Austral. Unidad Académica Caleta Olivia. Departamento de Ciencias Exactas y Naturales; Argentina
Materia
Asteroids: General
Minor Planets
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/72603
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Origin of slow-rotating minor bodies by tidal decoupling of binary pairsBrunini, AdrianAsteroids: GeneralMinor Planetshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this paper, we show that the decoupling of binary pairs by tidal interaction and Kozai oscillations acting together can generate single objects in a slow-rotation-rate state. This mechanism has the merit of not being strongly dependent on the size or shape of the objects. The key parameter leading the process is ω/n, the ratio between the rotation rate and the orbital mean motion of the binary, which must be > 1. The proposed mechanism could also operate in other populations of minor bodies.Fil: Brunini, Adrian. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de la Patagonia Austral. Unidad Académica Caleta Olivia. Departamento de Ciencias Exactas y Naturales; ArgentinaWiley Blackwell Publishing, Inc2017-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/72603Brunini, Adrian; Origin of slow-rotating minor bodies by tidal decoupling of binary pairs; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 465; 4; 3-2017; 3949-39550035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/465/4/3949/2568841?redirectedFrom=fulltextinfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw3043info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:33:30Zoai:ri.conicet.gov.ar:11336/72603instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:33:30.712CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Origin of slow-rotating minor bodies by tidal decoupling of binary pairs
title Origin of slow-rotating minor bodies by tidal decoupling of binary pairs
spellingShingle Origin of slow-rotating minor bodies by tidal decoupling of binary pairs
Brunini, Adrian
Asteroids: General
Minor Planets
title_short Origin of slow-rotating minor bodies by tidal decoupling of binary pairs
title_full Origin of slow-rotating minor bodies by tidal decoupling of binary pairs
title_fullStr Origin of slow-rotating minor bodies by tidal decoupling of binary pairs
title_full_unstemmed Origin of slow-rotating minor bodies by tidal decoupling of binary pairs
title_sort Origin of slow-rotating minor bodies by tidal decoupling of binary pairs
dc.creator.none.fl_str_mv Brunini, Adrian
author Brunini, Adrian
author_facet Brunini, Adrian
author_role author
dc.subject.none.fl_str_mv Asteroids: General
Minor Planets
topic Asteroids: General
Minor Planets
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In this paper, we show that the decoupling of binary pairs by tidal interaction and Kozai oscillations acting together can generate single objects in a slow-rotation-rate state. This mechanism has the merit of not being strongly dependent on the size or shape of the objects. The key parameter leading the process is ω/n, the ratio between the rotation rate and the orbital mean motion of the binary, which must be > 1. The proposed mechanism could also operate in other populations of minor bodies.
Fil: Brunini, Adrian. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de la Patagonia Austral. Unidad Académica Caleta Olivia. Departamento de Ciencias Exactas y Naturales; Argentina
description In this paper, we show that the decoupling of binary pairs by tidal interaction and Kozai oscillations acting together can generate single objects in a slow-rotation-rate state. This mechanism has the merit of not being strongly dependent on the size or shape of the objects. The key parameter leading the process is ω/n, the ratio between the rotation rate and the orbital mean motion of the binary, which must be > 1. The proposed mechanism could also operate in other populations of minor bodies.
publishDate 2017
dc.date.none.fl_str_mv 2017-03
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
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://hdl.handle.net/11336/72603
Brunini, Adrian; Origin of slow-rotating minor bodies by tidal decoupling of binary pairs; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 465; 4; 3-2017; 3949-3955
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/72603
identifier_str_mv Brunini, Adrian; Origin of slow-rotating minor bodies by tidal decoupling of binary pairs; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 465; 4; 3-2017; 3949-3955
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/465/4/3949/2568841?redirectedFrom=fulltext
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw3043
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 12.982451

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