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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/ |
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author | Kozai, Yoshihide |
author_facet | Kozai, Yoshihide |
author_sort | Kozai, Yoshihide |
collection | PubMed |
description | 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 seems to be consistent with numerical results published in various papers on subjects like periodic comets, planets of extra-solar systems, star clusters and binaries of black-holes. |
format | Online Article Text |
id | pubmed-8153358 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2004 |
publisher | The Japan Academy |
record_format | MEDLINE/PubMed |
spelling | pubmed-81533582021-05-28 Extension of secular perturbation theory for asteroids Kozai, Yoshihide Proc Jpn Acad Ser B Phys Biol Sci Review 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 seems to be consistent with numerical results published in various papers on subjects like periodic comets, planets of extra-solar systems, star clusters and binaries of black-holes. The Japan Academy 2004-03 2004-04-01 /pmc/articles/PMC8153358/ Text en © 2004 The Japan Academy https://creativecommons.org/licenses/by/4.0/This is an open access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. |
spellingShingle | Review Kozai, Yoshihide Extension of secular perturbation theory for asteroids |
title | Extension of secular perturbation theory for asteroids |
title_full | Extension of secular perturbation theory for asteroids |
title_fullStr | Extension of secular perturbation theory for asteroids |
title_full_unstemmed | Extension of secular perturbation theory for asteroids |
title_short | Extension of secular perturbation theory for asteroids |
title_sort | extension of secular perturbation theory for asteroids |
topic | Review |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8153358/ |
work_keys_str_mv | AT kozaiyoshihide extensionofsecularperturbationtheoryforasteroids |