Improvement of the IAU 2006 precession model with an updated Earth's J2 long-term variation

Autores
Liu, J.- C.
Año de publicación
2025
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
At its 2006 General Assembly, IAU has adopted a standard precession theory, called the "IAU 2006 precession”. The linear variation of the Earth’s dynamical flattening J2 was considered for the precession rate in longitude. However, the uncertainty in the J2 model is one of the greatest sources of uncertainty in this precession theory. In this report, we use the latest observational data from the satellite laser ranging (SLR) to investigate the effect of J2 long-time variations in solving the precession of the equator. The polynomial expressions for precession quantities are developed with a method similar to the IAU 2006 approach and are checked using the latest VLBI observations. The newly developed precession solution is clearly more consistent with VLBI observations and can reduce most of the curvature signals in the CPO series. Since the improvement relative to the IAU 2006 precession model is quite significant, we propose that a serious study for updating the IAU precession be carried out by relevant IAU Working Groups.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
IAU 2006 precession
Earth dynamical flattening (J2)
Satellite Laser Ranging (SLR)
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:10915/192028

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spelling Improvement of the IAU 2006 precession model with an updated Earth's J2 long-term variationLiu, J.- C.Ciencias AstronómicasIAU 2006 precessionEarth dynamical flattening (J2)Satellite Laser Ranging (SLR)At its 2006 General Assembly, IAU has adopted a standard precession theory, called the "IAU 2006 precession”. The linear variation of the Earth’s dynamical flattening J2 was considered for the precession rate in longitude. However, the uncertainty in the J2 model is one of the greatest sources of uncertainty in this precession theory. In this report, we use the latest observational data from the satellite laser ranging (SLR) to investigate the effect of J2 long-time variations in solving the precession of the equator. The polynomial expressions for precession quantities are developed with a method similar to the IAU 2006 approach and are checked using the latest VLBI observations. The newly developed precession solution is clearly more consistent with VLBI observations and can reduce most of the curvature signals in the CPO series. Since the improvement relative to the IAU 2006 precession model is quite significant, we propose that a serious study for updating the IAU precession be carried out by relevant IAU Working Groups.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/10915/192028enginfo: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:UNLP2026-05-13T12:59:24Zoai:sedici.unlp.edu.ar:10915/192028Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-05-13 12:59:24.961SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Improvement of the IAU 2006 precession model with an updated Earth's J2 long-term variation
title Improvement of the IAU 2006 precession model with an updated Earth's J2 long-term variation
spellingShingle Improvement of the IAU 2006 precession model with an updated Earth's J2 long-term variation
Liu, J.- C.
Ciencias Astronómicas
IAU 2006 precession
Earth dynamical flattening (J2)
Satellite Laser Ranging (SLR)
title_short Improvement of the IAU 2006 precession model with an updated Earth's J2 long-term variation
title_full Improvement of the IAU 2006 precession model with an updated Earth's J2 long-term variation
title_fullStr Improvement of the IAU 2006 precession model with an updated Earth's J2 long-term variation
title_full_unstemmed Improvement of the IAU 2006 precession model with an updated Earth's J2 long-term variation
title_sort Improvement of the IAU 2006 precession model with an updated Earth's J2 long-term variation
dc.creator.none.fl_str_mv Liu, J.- C.
author Liu, J.- C.
author_facet Liu, J.- C.
author_role author
dc.subject.none.fl_str_mv Ciencias Astronómicas
IAU 2006 precession
Earth dynamical flattening (J2)
Satellite Laser Ranging (SLR)
topic Ciencias Astronómicas
IAU 2006 precession
Earth dynamical flattening (J2)
Satellite Laser Ranging (SLR)
dc.description.none.fl_txt_mv At its 2006 General Assembly, IAU has adopted a standard precession theory, called the "IAU 2006 precession”. The linear variation of the Earth’s dynamical flattening J2 was considered for the precession rate in longitude. However, the uncertainty in the J2 model is one of the greatest sources of uncertainty in this precession theory. In this report, we use the latest observational data from the satellite laser ranging (SLR) to investigate the effect of J2 long-time variations in solving the precession of the equator. The polynomial expressions for precession quantities are developed with a method similar to the IAU 2006 approach and are checked using the latest VLBI observations. The newly developed precession solution is clearly more consistent with VLBI observations and can reduce most of the curvature signals in the CPO series. Since the improvement relative to the IAU 2006 precession model is quite significant, we propose that a serious study for updating the IAU precession be carried out by relevant IAU Working Groups.
Facultad de Ciencias Astronómicas y Geofísicas
description At its 2006 General Assembly, IAU has adopted a standard precession theory, called the "IAU 2006 precession”. The linear variation of the Earth’s dynamical flattening J2 was considered for the precession rate in longitude. However, the uncertainty in the J2 model is one of the greatest sources of uncertainty in this precession theory. In this report, we use the latest observational data from the satellite laser ranging (SLR) to investigate the effect of J2 long-time variations in solving the precession of the equator. The polynomial expressions for precession quantities are developed with a method similar to the IAU 2006 approach and are checked using the latest VLBI observations. The newly developed precession solution is clearly more consistent with VLBI observations and can reduce most of the curvature signals in the CPO series. Since the improvement relative to the IAU 2006 precession model is quite significant, we propose that a serious study for updating the IAU precession be carried out by relevant IAU Working Groups.
publishDate 2025
dc.date.none.fl_str_mv 2025-08
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info:eu-repo/semantics/publishedVersion
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dc.language.none.fl_str_mv eng
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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)
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Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
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repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
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