Spin orientation of the Galilean satellites
- Autores
- Yseboodt, M.; Baland, R.M.; Van Hoolst, T.
- Año de publicación
- 2025
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- The Galilean satellites are locked in a 1:1 spin-orbit resonance. Their rotation axis is assumed to be in a Cassini state and to follow the long-term precession of the orbit normal. The obliquity, which is the angular separation between the rotation axis and the orbit normal, is expected to be small.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Orbit
Satellite
Orientation
Rotation - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-nd/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/192184
Ver los metadatos del registro completo
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Spin orientation of the Galilean satellitesYseboodt, M.Baland, R.M.Van Hoolst, T.Ciencias AstronómicasOrbitSatelliteOrientationRotationThe Galilean satellites are locked in a 1:1 spin-orbit resonance. Their rotation axis is assumed to be in a Cassini state and to follow the long-term precession of the orbit normal. The obliquity, which is the angular separation between the rotation axis and the orbit normal, is expected to be small.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/10915/192184enginfo: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:10915/192184Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-03-31 12:42:01.857SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Spin orientation of the Galilean satellites |
| title |
Spin orientation of the Galilean satellites |
| spellingShingle |
Spin orientation of the Galilean satellites Yseboodt, M. Ciencias Astronómicas Orbit Satellite Orientation Rotation |
| title_short |
Spin orientation of the Galilean satellites |
| title_full |
Spin orientation of the Galilean satellites |
| title_fullStr |
Spin orientation of the Galilean satellites |
| title_full_unstemmed |
Spin orientation of the Galilean satellites |
| title_sort |
Spin orientation of the Galilean satellites |
| dc.creator.none.fl_str_mv |
Yseboodt, M. Baland, R.M. Van Hoolst, T. |
| author |
Yseboodt, M. |
| author_facet |
Yseboodt, M. Baland, R.M. Van Hoolst, T. |
| author_role |
author |
| author2 |
Baland, R.M. Van Hoolst, T. |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Orbit Satellite Orientation Rotation |
| topic |
Ciencias Astronómicas Orbit Satellite Orientation Rotation |
| dc.description.none.fl_txt_mv |
The Galilean satellites are locked in a 1:1 spin-orbit resonance. Their rotation axis is assumed to be in a Cassini state and to follow the long-term precession of the orbit normal. The obliquity, which is the angular separation between the rotation axis and the orbit normal, is expected to be small. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
The Galilean satellites are locked in a 1:1 spin-orbit resonance. Their rotation axis is assumed to be in a Cassini state and to follow the long-term precession of the orbit normal. The obliquity, which is the angular separation between the rotation axis and the orbit normal, is expected to be small. |
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2025 |
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2025-08 |
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eng |
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eng |
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