The invariable plane of the solar system based on modern long-term ephemerides of the major, dwarf and minor planets

Autores
Kudryavtsev, S. M.
Año de publicación
2025
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
The invariable plane of a dynamical system is a plane perpendicular to the total angular momentum vector of the system and it passes through the system’s barycenter. The invariable plane of the solar system is one of the most "natural” reference planes used in many applications (e.g., [1]). In [2] the orientation parameters of such the plane were earlier derived. They are inclination and ascending node of the invariable plane w.r.t. either ICRS or equinox-ecliptic of the epoch J2000. To calculate the instantaneous angular momentum vector of the solar system, study [2] used the positions of the major planets from the DE405/406 and INPOP 10a numerical ephemerides. Additionally, the input from Pluto, (1) Ceres, (4) Vesta and (2) Pallas was taken into account.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
Solar system
Planets
Asteroids
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-nd/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/192138
Acceder
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network_name_str SEDICI (UNLP)
spelling The invariable plane of the solar system based on modern long-term ephemerides of the major, dwarf and minor planetsKudryavtsev, S. M.Ciencias AstronómicasSolar systemPlanetsAsteroidsThe invariable plane of a dynamical system is a plane perpendicular to the total angular momentum vector of the system and it passes through the system’s barycenter. The invariable plane of the solar system is one of the most "natural” reference planes used in many applications (e.g., [1]). In [2] the orientation parameters of such the plane were earlier derived. They are inclination and ascending node of the invariable plane w.r.t. either ICRS or equinox-ecliptic of the epoch J2000. To calculate the instantaneous angular momentum vector of the solar system, study [2] used the positions of the major planets from the DE405/406 and INPOP 10a numerical ephemerides. Additionally, the input from Pluto, (1) Ceres, (4) Vesta and (2) Pallas was taken into account.Facultad de Ciencias Astronómicas y Geofísicas2025-08info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionResumenhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/192138enginfo:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/190232info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-nd/4.0/Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2026-03-31T12:42:01Zoai:sedici.unlp.edu.ar:10915/192138Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-03-31 12:42:01.91SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv The invariable plane of the solar system based on modern long-term ephemerides of the major, dwarf and minor planets
title The invariable plane of the solar system based on modern long-term ephemerides of the major, dwarf and minor planets
spellingShingle The invariable plane of the solar system based on modern long-term ephemerides of the major, dwarf and minor planets
Kudryavtsev, S. M.
Ciencias Astronómicas
Solar system
Planets
Asteroids
title_short The invariable plane of the solar system based on modern long-term ephemerides of the major, dwarf and minor planets
title_full The invariable plane of the solar system based on modern long-term ephemerides of the major, dwarf and minor planets
title_fullStr The invariable plane of the solar system based on modern long-term ephemerides of the major, dwarf and minor planets
title_full_unstemmed The invariable plane of the solar system based on modern long-term ephemerides of the major, dwarf and minor planets
title_sort The invariable plane of the solar system based on modern long-term ephemerides of the major, dwarf and minor planets
dc.creator.none.fl_str_mv Kudryavtsev, S. M.
author Kudryavtsev, S. M.
author_facet Kudryavtsev, S. M.
author_role author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Solar system
Planets
Asteroids
topic Ciencias Astronómicas
Solar system
Planets
Asteroids
dc.description.none.fl_txt_mv The invariable plane of a dynamical system is a plane perpendicular to the total angular momentum vector of the system and it passes through the system’s barycenter. The invariable plane of the solar system is one of the most "natural” reference planes used in many applications (e.g., [1]). In [2] the orientation parameters of such the plane were earlier derived. They are inclination and ascending node of the invariable plane w.r.t. either ICRS or equinox-ecliptic of the epoch J2000. To calculate the instantaneous angular momentum vector of the solar system, study [2] used the positions of the major planets from the DE405/406 and INPOP 10a numerical ephemerides. Additionally, the input from Pluto, (1) Ceres, (4) Vesta and (2) Pallas was taken into account.
Facultad de Ciencias Astronómicas y Geofísicas
description The invariable plane of a dynamical system is a plane perpendicular to the total angular momentum vector of the system and it passes through the system’s barycenter. The invariable plane of the solar system is one of the most "natural” reference planes used in many applications (e.g., [1]). In [2] the orientation parameters of such the plane were earlier derived. They are inclination and ascending node of the invariable plane w.r.t. either ICRS or equinox-ecliptic of the epoch J2000. To calculate the instantaneous angular momentum vector of the solar system, study [2] used the positions of the major planets from the DE405/406 and INPOP 10a numerical ephemerides. Additionally, the input from Pluto, (1) Ceres, (4) Vesta and (2) Pallas was taken into account.
publishDate 2025
dc.date.none.fl_str_mv 2025-08
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info:eu-repo/semantics/publishedVersion
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dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/192138
url http://sedici.unlp.edu.ar/handle/10915/192138
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/190232
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
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Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-nd/4.0/
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dc.format.none.fl_str_mv application/pdf
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reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
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repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
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