Identification of Asteroids in Two-Body Resonances
- Авторы: Smirnov E.A.1, Dovgalev I.S.2
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Учреждения:
- Pulkovo Observatory
- 4xxi Ltd.
- Выпуск: Том 52, № 4 (2018)
- Страницы: 347-354
- Раздел: Article
- URL: https://journal-vniispk.ru/0038-0946/article/view/171043
- DOI: https://doi.org/10.1134/S0038094618040056
- ID: 171043
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Аннотация
A catalog of asteroids in two-body orbital resonances with the planets of the Solar System has been created. The AstDyS database was a source of the input data, and all the numbered objects (467303 objects at the time of the analysis) were considered. The orbits were integrated in the framework of a pure gravitational problem considering all the planets of the Solar System and Pluto. From the analysis of the behavior of the resonant argument and the semimajor axis on the 100-kyr interval, the resonance membership and the libration type (pure or transient) were verified for each of the asteroids. A more accurate method to identify the resonant argument librations was developed on the basis of the analysis of mutual periodograms. We found 23251 resonant asteroids, ~36% of which (8397 objects) are in pure resonances.
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Об авторах
E. Smirnov
Pulkovo Observatory
Автор, ответственный за переписку.
Email: smirik@gmail.com
Россия, St. Petersburg, 196140
I. Dovgalev
4xxi Ltd.
Email: smirik@gmail.com
Россия, St. Petersburg, 197101
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