Effect of a Non-Hydrostatic Core-Mantle Boundary on Earth's and Mars'Rotational Dynamics

Autores
Folgueira-López, M.; Dehant, V.; Puica, M.; Brekier, J.; Van Hoolst, T.
Año de publicación
2025
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Dynamic loads within planetary mantles can deform the core-mantle boundary (CMB). On Earth, subducting slabs primarily induce degree-2, order-2 deformation of the CMB, though additional degrees arise when expanded in spherical harmonics. Nutations, observed through Very Long Baseline Interferometry (VLBI), and variations in the Length of Day (LOD) are measured with high precision. While the first-order effect of Earth's nonhydrostatic flattening significantly contributes to nutation amplitudes, we focus here on second-order effects. We compute the pressure torque acting on an irregular CMB, which can perturb both nutations and LOD. For nutations, topographic effects are generally small, as they are proportional to the product of two topography coefficients, except in cases of resonance, where the tidal frequency is close to an inertial wave frequency. We identify three such cases, though none lead to nutation amplifications exceeding 2 microarcseconds. This finding definitely excludes topographic pressure as an efficient mechanism to explain nutations. For LOD, we find significant amplification near specific resonances: the tide at 13.633 days is quite close to an inertial wave at 13.614 days, and the tide at 27.555 days to an inertial wave at 27.666 days, both resulting in an amplification of 0.06 milliseconds, at the level of the observed residuals. We also assess the effects on Mars but find that its tidal and nutation frequencies do not come sufficiently close to the determined inertial wave frequencies, leading to negligible resonance effects.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
Core-mantle boundary (CMB) deformation
Nutation and Length of Day (LOD)
Tidal resonance effects
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:10915/191975

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spelling Effect of a Non-Hydrostatic Core-Mantle Boundary on Earth's and Mars'Rotational DynamicsFolgueira-López, M.Dehant, V.Puica, M.Brekier, J.Van Hoolst, T.Ciencias AstronómicasCore-mantle boundary (CMB) deformationNutation and Length of Day (LOD)Tidal resonance effectsDynamic loads within planetary mantles can deform the core-mantle boundary (CMB). On Earth, subducting slabs primarily induce degree-2, order-2 deformation of the CMB, though additional degrees arise when expanded in spherical harmonics. Nutations, observed through Very Long Baseline Interferometry (VLBI), and variations in the Length of Day (LOD) are measured with high precision. While the first-order effect of Earth's nonhydrostatic flattening significantly contributes to nutation amplitudes, we focus here on second-order effects. We compute the pressure torque acting on an irregular CMB, which can perturb both nutations and LOD. For nutations, topographic effects are generally small, as they are proportional to the product of two topography coefficients, except in cases of resonance, where the tidal frequency is close to an inertial wave frequency. We identify three such cases, though none lead to nutation amplifications exceeding 2 microarcseconds. This finding definitely excludes topographic pressure as an efficient mechanism to explain nutations. For LOD, we find significant amplification near specific resonances: the tide at 13.633 days is quite close to an inertial wave at 13.614 days, and the tide at 27.555 days to an inertial wave at 27.666 days, both resulting in an amplification of 0.06 milliseconds, at the level of the observed residuals. We also assess the effects on Mars but find that its tidal and nutation frequencies do not come sufficiently close to the determined inertial wave frequencies, leading to negligible resonance effects.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/pdf32-33http://sedici.unlp.edu.ar/handle/10915/191975enginfo: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:UNLP2026-03-26T09:21:46Zoai:sedici.unlp.edu.ar:10915/191975Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-03-26 09:21:46.972SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Effect of a Non-Hydrostatic Core-Mantle Boundary on Earth's and Mars'Rotational Dynamics
title Effect of a Non-Hydrostatic Core-Mantle Boundary on Earth's and Mars'Rotational Dynamics
spellingShingle Effect of a Non-Hydrostatic Core-Mantle Boundary on Earth's and Mars'Rotational Dynamics
Folgueira-López, M.
Ciencias Astronómicas
Core-mantle boundary (CMB) deformation
Nutation and Length of Day (LOD)
Tidal resonance effects
title_short Effect of a Non-Hydrostatic Core-Mantle Boundary on Earth's and Mars'Rotational Dynamics
title_full Effect of a Non-Hydrostatic Core-Mantle Boundary on Earth's and Mars'Rotational Dynamics
title_fullStr Effect of a Non-Hydrostatic Core-Mantle Boundary on Earth's and Mars'Rotational Dynamics
title_full_unstemmed Effect of a Non-Hydrostatic Core-Mantle Boundary on Earth's and Mars'Rotational Dynamics
title_sort Effect of a Non-Hydrostatic Core-Mantle Boundary on Earth's and Mars'Rotational Dynamics
dc.creator.none.fl_str_mv Folgueira-López, M.
Dehant, V.
Puica, M.
Brekier, J.
Van Hoolst, T.
author Folgueira-López, M.
author_facet Folgueira-López, M.
Dehant, V.
Puica, M.
Brekier, J.
Van Hoolst, T.
author_role author
author2 Dehant, V.
Puica, M.
Brekier, J.
Van Hoolst, T.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Core-mantle boundary (CMB) deformation
Nutation and Length of Day (LOD)
Tidal resonance effects
topic Ciencias Astronómicas
Core-mantle boundary (CMB) deformation
Nutation and Length of Day (LOD)
Tidal resonance effects
dc.description.none.fl_txt_mv Dynamic loads within planetary mantles can deform the core-mantle boundary (CMB). On Earth, subducting slabs primarily induce degree-2, order-2 deformation of the CMB, though additional degrees arise when expanded in spherical harmonics. Nutations, observed through Very Long Baseline Interferometry (VLBI), and variations in the Length of Day (LOD) are measured with high precision. While the first-order effect of Earth's nonhydrostatic flattening significantly contributes to nutation amplitudes, we focus here on second-order effects. We compute the pressure torque acting on an irregular CMB, which can perturb both nutations and LOD. For nutations, topographic effects are generally small, as they are proportional to the product of two topography coefficients, except in cases of resonance, where the tidal frequency is close to an inertial wave frequency. We identify three such cases, though none lead to nutation amplifications exceeding 2 microarcseconds. This finding definitely excludes topographic pressure as an efficient mechanism to explain nutations. For LOD, we find significant amplification near specific resonances: the tide at 13.633 days is quite close to an inertial wave at 13.614 days, and the tide at 27.555 days to an inertial wave at 27.666 days, both resulting in an amplification of 0.06 milliseconds, at the level of the observed residuals. We also assess the effects on Mars but find that its tidal and nutation frequencies do not come sufficiently close to the determined inertial wave frequencies, leading to negligible resonance effects.
Facultad de Ciencias Astronómicas y Geofísicas
description Dynamic loads within planetary mantles can deform the core-mantle boundary (CMB). On Earth, subducting slabs primarily induce degree-2, order-2 deformation of the CMB, though additional degrees arise when expanded in spherical harmonics. Nutations, observed through Very Long Baseline Interferometry (VLBI), and variations in the Length of Day (LOD) are measured with high precision. While the first-order effect of Earth's nonhydrostatic flattening significantly contributes to nutation amplitudes, we focus here on second-order effects. We compute the pressure torque acting on an irregular CMB, which can perturb both nutations and LOD. For nutations, topographic effects are generally small, as they are proportional to the product of two topography coefficients, except in cases of resonance, where the tidal frequency is close to an inertial wave frequency. We identify three such cases, though none lead to nutation amplifications exceeding 2 microarcseconds. This finding definitely excludes topographic pressure as an efficient mechanism to explain nutations. For LOD, we find significant amplification near specific resonances: the tide at 13.633 days is quite close to an inertial wave at 13.614 days, and the tide at 27.555 days to an inertial wave at 27.666 days, both resulting in an amplification of 0.06 milliseconds, at the level of the observed residuals. We also assess the effects on Mars but find that its tidal and nutation frequencies do not come sufficiently close to the determined inertial wave frequencies, leading to negligible resonance effects.
publishDate 2025
dc.date.none.fl_str_mv 2025-08
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Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
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