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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Autor principal: Riú, Pedro Carlos
Formato: Articulo
Lenguaje:Español
Publicado: 1963
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/90968
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spelling 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
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