Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide
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 differ...
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| Formato: | Articulo |
| Lenguaje: | Español |
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1963
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/90968 |
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I19-R120-10915-90968 |
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I19-R120-10915-909682024-06-05T18:53:20Z http://sedici.unlp.edu.ar/handle/10915/90968 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 Riú, Pedro Carlos 1963 2020-03-17T12:51:44Z es Ciencias Astronómicas función perturbadora 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 Articulo Articulo http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 50-60 |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Español |
| topic |
Ciencias Astronómicas función perturbadora |
| spellingShingle |
Ciencias Astronómicas función perturbadora Riú, Pedro Carlos Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide |
| topic_facet |
Ciencias Astronómicas función perturbadora |
| 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. |
| format |
Articulo Articulo |
| author |
Riú, Pedro Carlos |
| author_facet |
Riú, Pedro Carlos |
| author_sort |
Riú, Pedro Carlos |
| title |
Cálculo de las perturbaciones de la anomalía media y del radio vector de un asteroide |
| 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 |
| publishDate |
1963 |
| url |
http://sedici.unlp.edu.ar/handle/10915/90968 |
| work_keys_str_mv |
AT riupedrocarlos calculodelasperturbacionesdelaanomaliamediaydelradiovectordeunasteroide AT riupedrocarlos calculationoftheperturbationsofthemeananomalyandtheradiusvectorofanasteroid |
| _version_ |
1807220477112877056 |