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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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Formato: | Online Artículo Texto |
Lenguaje: | English |
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The Japan Academy
2004
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Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8153358/ |