A statistically sound model for astrometric uncertainties to improve minor planet orbit accuracies
- Autores
- Spoto, F.; Payne, M.; Holman, M.
- Año de publicación
- 2025
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- Astrometric uncertainties are central to any orbit-fitting procedure. The result of a fit is a nominal solution, which represents the single orbit that best matches the observations, and a confidence region describing the orbital uncertainty, which includes the set of orbital elements statistically compatible with the data and the error model. For well-observed asteroids, the region is well approximated by a multidimensional ellipsoid. In contrast, for short-arc objects (e.g. objects on the NEO Confirmation Page), the uncertainty region appears as a cloud of admissible orbits.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Orbital uncertainty
Astrometric errors
Statistical error model - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-nd/4.0/
- Repositorio
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- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/192137
Ver los metadatos del registro completo
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A statistically sound model for astrometric uncertainties to improve minor planet orbit accuraciesSpoto, F.Payne, M.Holman, M.Ciencias AstronómicasOrbital uncertaintyAstrometric errorsStatistical error modelAstrometric uncertainties are central to any orbit-fitting procedure. The result of a fit is a nominal solution, which represents the single orbit that best matches the observations, and a confidence region describing the orbital uncertainty, which includes the set of orbital elements statistically compatible with the data and the error model. For well-observed asteroids, the region is well approximated by a multidimensional ellipsoid. In contrast, for short-arc objects (e.g. objects on the NEO Confirmation Page), the uncertainty region appears as a cloud of admissible orbits.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/10915/192137enginfo: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:UNLP2026-04-15T11:59:04Zoai:sedici.unlp.edu.ar:10915/192137Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-04-15 11:59:05.015SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
A statistically sound model for astrometric uncertainties to improve minor planet orbit accuracies |
| title |
A statistically sound model for astrometric uncertainties to improve minor planet orbit accuracies |
| spellingShingle |
A statistically sound model for astrometric uncertainties to improve minor planet orbit accuracies Spoto, F. Ciencias Astronómicas Orbital uncertainty Astrometric errors Statistical error model |
| title_short |
A statistically sound model for astrometric uncertainties to improve minor planet orbit accuracies |
| title_full |
A statistically sound model for astrometric uncertainties to improve minor planet orbit accuracies |
| title_fullStr |
A statistically sound model for astrometric uncertainties to improve minor planet orbit accuracies |
| title_full_unstemmed |
A statistically sound model for astrometric uncertainties to improve minor planet orbit accuracies |
| title_sort |
A statistically sound model for astrometric uncertainties to improve minor planet orbit accuracies |
| dc.creator.none.fl_str_mv |
Spoto, F. Payne, M. Holman, M. |
| author |
Spoto, F. |
| author_facet |
Spoto, F. Payne, M. Holman, M. |
| author_role |
author |
| author2 |
Payne, M. Holman, M. |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Orbital uncertainty Astrometric errors Statistical error model |
| topic |
Ciencias Astronómicas Orbital uncertainty Astrometric errors Statistical error model |
| dc.description.none.fl_txt_mv |
Astrometric uncertainties are central to any orbit-fitting procedure. The result of a fit is a nominal solution, which represents the single orbit that best matches the observations, and a confidence region describing the orbital uncertainty, which includes the set of orbital elements statistically compatible with the data and the error model. For well-observed asteroids, the region is well approximated by a multidimensional ellipsoid. In contrast, for short-arc objects (e.g. objects on the NEO Confirmation Page), the uncertainty region appears as a cloud of admissible orbits. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
Astrometric uncertainties are central to any orbit-fitting procedure. The result of a fit is a nominal solution, which represents the single orbit that best matches the observations, and a confidence region describing the orbital uncertainty, which includes the set of orbital elements statistically compatible with the data and the error model. For well-observed asteroids, the region is well approximated by a multidimensional ellipsoid. In contrast, for short-arc objects (e.g. objects on the NEO Confirmation Page), the uncertainty region appears as a cloud of admissible orbits. |
| publishDate |
2025 |
| dc.date.none.fl_str_mv |
2025-08 |
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info:eu-repo/semantics/conferenceObject info:eu-repo/semantics/publishedVersion Resumen http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
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conferenceObject |
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http://sedici.unlp.edu.ar/handle/10915/192137 |
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eng |
| language |
eng |
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info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/190232 |
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openAccess |
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