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Libration Points of Triaxial Rotating Ellipsoid and their Application in Geodynamics

  • Askar Bekov
Conference paper
Part of the NATO ASI Series book series (ASEN, volume 4)

Abstract

The development of the modern and perspective methods and means of celestial mechanics and satellite geodesy using the results of observations and measurings with the help of artificial satellites and cosmic apparatus offer the possibility to obtain high-exact atsronomo-geodesical information on structure of the Earth’s external gravitational field, the specification of the Earth’s size and form, the definition and the specification of the observation points coordinates on the Earth.

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References

  1. Bekov AA (1990) On the Hill surface near the rotating nonstationary triaxialo ellipsoid. Izvestia AN Kazakh SSR 4: 49–52Google Scholar
  2. Bekov AA (1992) On the motion of the test body near the gravitating triaxial ellipsoid in rotating with variable physical parameters. Problems of the dynamics of the stellar systems Alma-Ata 50: 45–61Google Scholar
  3. Bursa M (1987) Secular deceleration of the Moon and of the Earth’s rotation and variation in the zonal geopotential harmonic. Bull. Atron. Inst. Czechoslovakia 38: 309–313Google Scholar
  4. Marchenko AN (1992) The determination of the some geodynamical parameters from observations of the artificial satellites “Lageos”and “Etalon-1”. Kinemat. & Phys. celest. bodies 8: 81–88Google Scholar

Copyright information

© Springer-VerlagBerlin Heidelberg 1995

Authors and Affiliations

  • Askar Bekov
    • 1
  1. 1.Astrophysical InstituteKazakhstan

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