Skip to main content
Log in

On the true circular orbit of a satellite

  • Published:
Celestial mechanics Aims and scope Submit manuscript

Abstract

The osculating orbit of a planetary satellite moving in the equatorial plane of the central body under the influence of a rotational symmetric perturbation force is elliptical in first order approximation even if the true orbit is always circular. The satellite motion is influenced by a resonance effect due to this perturbing force. An inclined true satellite orbit cannot be circular.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Brouwer, D. and Clemence, G. M.: 1961,Methods of Celestial Mechanics, Academic Press, New York and London.

    Google Scholar 

  • Chebotarev, G. S.: 1967,Analytical and Numerical Methods of Celestial Mechanics, American Elsevier Publishing Company, Inc., New York.

    Google Scholar 

  • Flury, W.: 1973, ‘Station Keeping of a Geostationary Satellite’, ELDO-CECLES/ESRO-CERS Scient. and Techn. Rev. 5, 131–156.

    Google Scholar 

  • Flury, W.: 1976, ‘The Drift of a Near-Geostationary Satellite’, ESOC, IHD-M.A.D. Working Paper No. 12.

  • Kozai, Y.: 1959,Astron. J. 64, 367.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Jochim, E.F., Eckstein, M.C. On the true circular orbit of a satellite. Celestial Mechanics 21, 149–153 (1980). https://doi.org/10.1007/BF01230890

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01230890

Keywords

Navigation