Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide
- Autores
- Riú, Pedro Carlos
- Año de publicación
- 1963
- Idioma
- español castellano
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The classical disturbing function R is not suitable to most of the asteroids because in the integration of R, the very small divisor (k_1 n + k_2 n'), in the case -k_1/k_2 ~ n'/n, gives origin to a very large period inequality. In order to avoid such a difficulty, we have solved the differential equation of the Hansen-Bohlin method, by means of trigonometrical series using as independent variable ζ= A ∫ A_0 ^-3 (t) dt, instead of the eccentric anomaly. We used an analytical method and an application is made in the particular case of asteroid Thule for whicn n'/n ~ 3/4.
Asociación Argentina de Astronomía - Materia
-
Ciencias Astronómicas
función perturbadora - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/90968
Ver los metadatos del registro completo
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Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroideCalculation of the perturbations of the mean anomaly and the radius vector of an asteroidRiú, Pedro CarlosCiencias Astronómicasfunción perturbadoraThe classical disturbing function R is not suitable to most of the asteroids because in the integration of R, the very small divisor (k_1 n + k_2 n'), in the case -k_1/k_2 ~ n'/n, gives origin to a very large period inequality. In order to avoid such a difficulty, we have solved the differential equation of the Hansen-Bohlin method, by means of trigonometrical series using as independent variable ζ= A ∫ A_0 ^-3 (t) dt, instead of the eccentric anomaly. We used an analytical method and an application is made in the particular case of asteroid Thule for whicn n'/n ~ 3/4.Asociación Argentina de Astronomía1963info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf50-60http://sedici.unlp.edu.ar/handle/10915/90968spainfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T10:51:21Zoai:sedici.unlp.edu.ar:10915/90968Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:51:21.613SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide Calculation of the perturbations of the mean anomaly and the radius vector of an asteroid |
| title |
Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide |
| spellingShingle |
Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide Riú, Pedro Carlos Ciencias Astronómicas función perturbadora |
| title_short |
Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide |
| title_full |
Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide |
| title_fullStr |
Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide |
| title_full_unstemmed |
Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide |
| title_sort |
Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide |
| dc.creator.none.fl_str_mv |
Riú, Pedro Carlos |
| author |
Riú, Pedro Carlos |
| author_facet |
Riú, Pedro Carlos |
| author_role |
author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas función perturbadora |
| topic |
Ciencias Astronómicas función perturbadora |
| dc.description.none.fl_txt_mv |
The classical disturbing function R is not suitable to most of the asteroids because in the integration of R, the very small divisor (k_1 n + k_2 n'), in the case -k_1/k_2 ~ n'/n, gives origin to a very large period inequality. In order to avoid such a difficulty, we have solved the differential equation of the Hansen-Bohlin method, by means of trigonometrical series using as independent variable ζ= A ∫ A_0 ^-3 (t) dt, instead of the eccentric anomaly. We used an analytical method and an application is made in the particular case of asteroid Thule for whicn n'/n ~ 3/4. Asociación Argentina de Astronomía |
| description |
The classical disturbing function R is not suitable to most of the asteroids because in the integration of R, the very small divisor (k_1 n + k_2 n'), in the case -k_1/k_2 ~ n'/n, gives origin to a very large period inequality. In order to avoid such a difficulty, we have solved the differential equation of the Hansen-Bohlin method, by means of trigonometrical series using as independent variable ζ= A ∫ A_0 ^-3 (t) dt, instead of the eccentric anomaly. We used an analytical method and an application is made in the particular case of asteroid Thule for whicn n'/n ~ 3/4. |
| publishDate |
1963 |
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1963 |
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