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...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autor principal: Riú, Pedro Carlos
Formato: Articulo
Lenguaje:Español
Publicado: 1963
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/90968
Aporte de:

Ejemplares similares