On some aspects of the stirring rate of planetesimal velocities by a protoplanet
- Autores
- Brunini, Adrian; Santamaria, Pablo Javier
- Año de publicación
- 2007
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We discuss some aspects of the evolution of the relative velocities of a swarm of planetesimals stirred by a protoplanet. We show that the prescriptions most commonly used in semi-analytical ‘oligarchic growth’ models overestimate the relative velocities of planetesimals by a nonnegligible factor. We discuss the probable origin of this discrepancy, proposing a correction factor that provides good agreement between these prescriptions and the results of numerical experiments. The proposed correction factor can be easily implemented in semi-analytical accretion models
Fil: Brunini, Adrian. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Santamaria, Pablo Javier. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina - Materia
-
Solar system
Dynamics
Numerical simulations
Celestial mechanics - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/44107
Ver los metadatos del registro completo
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On some aspects of the stirring rate of planetesimal velocities by a protoplanetBrunini, AdrianSantamaria, Pablo JavierSolar systemDynamicsNumerical simulationsCelestial mechanicshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We discuss some aspects of the evolution of the relative velocities of a swarm of planetesimals stirred by a protoplanet. We show that the prescriptions most commonly used in semi-analytical ‘oligarchic growth’ models overestimate the relative velocities of planetesimals by a nonnegligible factor. We discuss the probable origin of this discrepancy, proposing a correction factor that provides good agreement between these prescriptions and the results of numerical experiments. The proposed correction factor can be easily implemented in semi-analytical accretion modelsFil: Brunini, Adrian. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Santamaria, Pablo Javier. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaWiley Blackwell Publishing, Inc2007-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/44107Brunini, Adrian; Santamaria, Pablo Javier; On some aspects of the stirring rate of planetesimal velocities by a protoplanet; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 378; 12-2007; 657-6610035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2007.11805.xinfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/378/2/657/961229info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-11-12T09:56:32Zoai:ri.conicet.gov.ar:11336/44107instacron: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:34982025-11-12 09:56:32.549CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
On some aspects of the stirring rate of planetesimal velocities by a protoplanet |
| title |
On some aspects of the stirring rate of planetesimal velocities by a protoplanet |
| spellingShingle |
On some aspects of the stirring rate of planetesimal velocities by a protoplanet Brunini, Adrian Solar system Dynamics Numerical simulations Celestial mechanics |
| title_short |
On some aspects of the stirring rate of planetesimal velocities by a protoplanet |
| title_full |
On some aspects of the stirring rate of planetesimal velocities by a protoplanet |
| title_fullStr |
On some aspects of the stirring rate of planetesimal velocities by a protoplanet |
| title_full_unstemmed |
On some aspects of the stirring rate of planetesimal velocities by a protoplanet |
| title_sort |
On some aspects of the stirring rate of planetesimal velocities by a protoplanet |
| dc.creator.none.fl_str_mv |
Brunini, Adrian Santamaria, Pablo Javier |
| author |
Brunini, Adrian |
| author_facet |
Brunini, Adrian Santamaria, Pablo Javier |
| author_role |
author |
| author2 |
Santamaria, Pablo Javier |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Solar system Dynamics Numerical simulations Celestial mechanics |
| topic |
Solar system Dynamics Numerical simulations Celestial mechanics |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
We discuss some aspects of the evolution of the relative velocities of a swarm of planetesimals stirred by a protoplanet. We show that the prescriptions most commonly used in semi-analytical ‘oligarchic growth’ models overestimate the relative velocities of planetesimals by a nonnegligible factor. We discuss the probable origin of this discrepancy, proposing a correction factor that provides good agreement between these prescriptions and the results of numerical experiments. The proposed correction factor can be easily implemented in semi-analytical accretion models Fil: Brunini, Adrian. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Santamaria, Pablo Javier. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina |
| description |
We discuss some aspects of the evolution of the relative velocities of a swarm of planetesimals stirred by a protoplanet. We show that the prescriptions most commonly used in semi-analytical ‘oligarchic growth’ models overestimate the relative velocities of planetesimals by a nonnegligible factor. We discuss the probable origin of this discrepancy, proposing a correction factor that provides good agreement between these prescriptions and the results of numerical experiments. The proposed correction factor can be easily implemented in semi-analytical accretion models |
| publishDate |
2007 |
| dc.date.none.fl_str_mv |
2007-12 |
| 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/11336/44107 Brunini, Adrian; Santamaria, Pablo Javier; On some aspects of the stirring rate of planetesimal velocities by a protoplanet; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 378; 12-2007; 657-661 0035-8711 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/44107 |
| identifier_str_mv |
Brunini, Adrian; Santamaria, Pablo Javier; On some aspects of the stirring rate of planetesimal velocities by a protoplanet; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 378; 12-2007; 657-661 0035-8711 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2007.11805.x info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/378/2/657/961229 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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Wiley Blackwell Publishing, Inc |
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Wiley Blackwell Publishing, Inc |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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