Celestial mechanics

, Volume 27, Issue 4, pp 325–337 | Cite as

On eccentricity functions for eccentric orbits

  • A. Szeto
  • K. Lambeck
Article

Abstract

Situations arise in celestial mechanics where orbital eccentricities are large and yet it is desirable to maintain the Darwin-Kaula Fourier decomposition of the perturbing function. Evaluation of the appropriate eccentricity functionsG lpq (e) requires a double summation which, for practical purposes, must be truncated. In this note criteria have been established for truncation of the expansion for eccentricities ≦0.75.

Keywords

Fourier Practical Purpose Celestial Mechanic Eccentric Orbit Fourier Decomposition 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Allan, R. R.: 1971, ‘Commensurable Eccentric Orbits Near Critical Inclination’,Celest. Mech. 3, 320.Google Scholar
  2. Charlier, C. L.: 1907,Die Mechanik des Himmels Bd2, Verlag von Veit and Co., Leipzig.Google Scholar
  3. Cherniack, J. R.: 1972, ‘Computation of Hansen Coefficients’,Smithson. Astrophys. Obs. Spec. Rep. 346.Google Scholar
  4. Cook, G. E.: 1973, ‘Basic Theory for PROD, a Program for Computing the Development of Satellite Orbits’,Celest. Mech. 7, 301.Google Scholar
  5. Gaposchkin, E. M.: 1973, ‘Satellite Dynamics’,Smithson. Astrophys. Obs. Spec. Rep. 353, 89.Google Scholar
  6. Gerstenkorn, H.: 1955, ‘Über Gezeitenreibung beim Zweikörperproblem’,Z. Astrophys. 36, 254.Google Scholar
  7. Goldreich, P.: 1966, ‘History of the Lunar Orbit’,Rev. Geophys. 4, 411.Google Scholar
  8. Hagihara, Y.: 1972,Celestial Mechanics, Vol. 1, MIT Press, Cambridge, Mass.Google Scholar
  9. Kaula, W. M.: 1964, ‘Tidal Dissipation by Solid Friction and the Resulting Orbital Evolution’,Rev. Geophys. 2, 661.Google Scholar
  10. Kaula, W. M.: 1966,Introduction to Satellite Geodesy, Blaisdell Publ. Co., Waltham, Mass.Google Scholar
  11. Kovalevsky, J.: 1967,Introduction to Celestial Mechanics, D. Reidel Publ. Co., Dordrecht, Holland.Google Scholar
  12. Kovalevsky, J. and Sagnier, J. L.: 1977, ‘Motions of Natural Satellites’, in J. Burns (ed.),Planetary Satellites, University of Arizona Press, Tuscon, Ariz.Google Scholar
  13. Lambeck, K.: 1979, ‘On the Orbital Evolution of the Martian Satellites’,J. Geophys. Res. 84, 5651.Google Scholar
  14. Lambeck, K.: 1980,The Earth's Variable Rotation; Geophysical Causes and Consequences, Cambridge University Press, Cambridge, U.K.Google Scholar
  15. Laplace, P. S.: 1830,Méchanique Céleste 5, Supplément.Google Scholar
  16. MacDonald, G. J. F.: 1964, ‘Tidal Friction’,Rev. Geophys. 2, 467.Google Scholar
  17. Mignard, F.: 1978, ‘Multiple Expansion of the Tidal Potential’,Celest. Mech. 18, 287.Google Scholar
  18. Plummer, H. C.: 1960,An Introductory Treatise on Dynamicals Astronomy, Dover Publ., N. Y. (originally published in 1912).Google Scholar
  19. Tisserand, F.: 1960,Traité du Méchanique Céleste, Vol. 1, Gauthier-Villars, Paris (originally published in 1896).Google Scholar
  20. Whittaker, E. T. and Watson, G. N.: 1963,A Course of Modern Analysis, 4th Ed., Cambridge Univ. Press, London.Google Scholar

Copyright information

© D. Reidel Publishing Co. 1982

Authors and Affiliations

  • A. Szeto
    • 1
  • K. Lambeck
    • 1
  1. 1.Research School of Earth SciencesAustralian National UniversityCanberraAustralia

Personalised recommendations