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Extension of secular perturbation theory for asteroids

In this paper the theory of secular perturbations of asteroids with high inclinations and eccentricities (1962) is reviewed and extended analytically for orbits of Kuiper-belt objects and the problem of stellar three bodies consisting of a binary and a distant third body. The theory thus extended se...

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Detalles Bibliográficos
Autor principal: Kozai, Yoshihide
Formato: Online Artículo Texto
Lenguaje:English
Publicado: The Japan Academy 2004
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8153358/