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14: Teoría general de la perturbación

Última actualización

30 oct 2022
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- 13.17: Observaciones finales
- 14.1: Introducción a la Teoría General de la Perturbación

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14.1: Introducción a la Teoría General de la Perturbación
14.2: Transformaciones de contacto y teoría de perturbación general
14.3: Los soportes de Poisson para los elementos orbitales
14.4: Ecuaciones Planetarias de Lagrange
Las ecuaciones planetarias de Lagrange nos permiten calcular las tasas de cambio de los elementos orbitales si conocemos la forma de la función perturbadora.
14.5: Movimiento alrededor de una cima simétrica oblata

Miniaturas: Animación que muestra la relación entre los cinco puntos lagrangianos (rojos) de un planeta (azul) orbitando una estrella (amarillo), y el potencial gravitacional en el plano que contiene la órbita (superficie gris con contornos morados de igual potencial). (CC BY-SA 4.0; cmglee).

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