Hostname: page-component-5cf477f64f-r2nwp Total loading time: 0 Render date: 2025-04-02T07:02:46.434Z Has data issue: false hasContentIssue false
  • English
  • Français

New semi-analytical calculation of lunar, solar and planetary perturbations in motion of Earth satellites

Published online by Cambridge University Press:  16 October 2024

Sergey M. Kudryavtsev Open the ORCID record for Sergey M. Kudryavtsev [Opens in a new window]
Sergey M. Kudryavtsev*
Affiliation:
M.V. Lomonosov Moscow State University, Sternberg Astronomical Institute, 13, Universitetsky Pr., Moscow, Russia
*
email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We suggest an advanced algorithm for semi-analytical calculation of orbital perturbations of Earth artificial satellites caused by the gravity attraction of the “3rd-bodies” (the Moon, the Sun, major planets). A new accurate analytical series for the relevant perturbation function is developed. It is obtained through a careful spectral analysis of the long-term DE406 planetary/lunar ephemerides and valid over 2000 years, 1000-3000. The series is used in the author’s semi-analytical model of satellite motion. The results of the motion prediction of several Earth satellites obtained by means of the semi-analytical model and a numerical integration method are compared.

Keywords

Satellite MotionSemi-Analytical ModelPerturbationsSunMoonMajor Planets
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S382: Complex Planetary Systems II: Latest Methods for an Interdisciplinary Approach , December 2022 , pp. 142 - 145
Check for updates
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

Emelyanov, N. V. 1980, Trudy GAISH, 49, 122 [in Russian]Google Scholar
Giacagalia, G. E. O. 1974, Celest. Mech., 9, 239 CrossRefGoogle Scholar
Ivanov, N. M., Kolyuka, Yu. F., Kudryavtsev, S. M., Tikhonov, V. F. 1988, Sov. Astron. Lett., 14, 405 Google Scholar
Kolyuka, Yu. F., Kudryavtsev, S. M., Tarasov, V. P., et al. 1991, Planet. Space Sci., 39, 349 CrossRefGoogle Scholar
Kudryavtsev, S. M. 1995, Celest. Mech. Dyn. Astron., 61, 207 CrossRefGoogle Scholar
Kudryavtsev, S. M. 1997, Celest. Mech. Dyn. Astron., 67, 131 CrossRefGoogle Scholar
Kudryavtsev, S. M. 2002, Celest. Mech. Dyn. Astron., 82, 301 CrossRefGoogle Scholar
Kudryavtsev, S. M. 2004, J. Geodesy, 77, 829 CrossRefGoogle Scholar
Kudryavtsev, S. M. 2007, A&A, 471, 1069 Google Scholar
Simon, J.-L., Bretagnon, P., Chapront, J., et al. 1994, A&A, 282, 663 Google Scholar
Standish, E. M. 1998, JPL Interoffice Memorandum, 312.F–98–048Google Scholar
Supplementary material: PDF

Kudryavtsev supplementary material

Kudryavtsev supplementary material

Download Kudryavtsev supplementary material(PDF)
PDF 53.1 KB