Consideration of Relativistic Effects in the Rotation of Mars and its Satellites
- Авторы: Pashkevich V.V.1, Vershkov A.V.1
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Учреждения:
- Central (Pulkovo) Astronomical Observatory, Russian Academy of Sciences
- Выпуск: Том 53, № 6 (2019)
- Страницы: 431-435
- Раздел: Article
- URL: https://journal-vniispk.ru/0038-0946/article/view/171404
- DOI: https://doi.org/10.1134/S0038094619060066
- ID: 171404
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Аннотация
This study is dedicated to the consideration of the relativistic effects (geodetic precession and nutation that make up the geodetic rotation) in the rotation of Mars and its satellites (Phobos and Deimos). The relativistic effects were calculated using the method developed in (Pashkevich, 2016), which is applicable to the study of any bodies of the Solar System that have long-term ephemerides. As a result, the most significant secular and periodic terms of the geodetic rotation in the perturbing terms of physical libration and in the Euler angles were determined for the Martian satellites for the first time.
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Об авторах
V. Pashkevich
Central (Pulkovo) Astronomical Observatory, Russian Academy of Sciences
Автор, ответственный за переписку.
Email: apeks@gaoran.ru
Россия, St. Petersburg
A. Vershkov
Central (Pulkovo) Astronomical Observatory, Russian Academy of Sciences
Email: apeks@gaoran.ru
Россия, St. Petersburg
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