Skip to main content
Log in

Satellite prediction formulae for Vinti's model

  • Published:
Celestial mechanics Aims and scope Submit manuscript

Abstract

For Vinti's dynamical problem, there is proposed a new form of solution wherein all three coordinates are expressed in terms of one independent variable. The formulae for the three co-ordinates are clear generalizations of the corresponding formulae for the Kepler problem while the independent variable corresponds to the true anomaly. The solution is completed by the relation connecting the independent variable with time: the latter is a generalization of the well known Kepler time-angle relationship. From the form and method of solution the main qualitative features of the motion are readily derived.

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

  • Aksenov, E. P., Gribenikov, E. A., and Demin, V. C.: 1964,Soviet Astron. 16, 164–174.

    Google Scholar 

  • Brouwer, D. and Clemence, G. M.: 1962,Methods of Celestial Mechanics, Academic Press, New York.

    Google Scholar 

  • Davis, H. T.: 1960,Introduction to Nonlinear Differential and Integral Equations, U.S. Govt. Printing Office, Washington, D.C.

    Google Scholar 

  • Izsak, I. M.: 1960, ‘A Theory of Satellite Motion about an Oblate Planet’, Smithsonian Institute Astrophysical Observatory, Research in Space Science, Special Report No. 52.

  • O'Mathuna, D.: 1969, The Vinti Dynamical Problem and the Geopotential. NASA TR R-307, ERC, Cambridge, Mass.

    Google Scholar 

  • Vinti, J. P.: 1959, ‘A New Method of Solution for Unretarded Satellite Orbits’,J. Res. NBS 63B;Math. Math. Phys. 2, 1965–116.

    Google Scholar 

  • Vinti, J. P.: 1961, ‘Theory of an Accurate Intermediary Orbit for Satellite Astronomy,J. Res. NBS 65B;Math. Math. Phys. 3, 169–201.

    Google Scholar 

  • Vinti, J. P.: 1963, ‘Zonal Harmonic Perturbations of an Accurate Reference Orbit of an Artificial Satellite’,J. Res. NBS 67B;Math. Math. Phys. 4, 191–222.

    Google Scholar 

  • Vinti, J. P.: 1966a, ‘Invariant Properties of the Spheroidal Potential of an Oblate Planet and Inclusion of the Third Zonal Harmonic in an Accurate Reference Orbit of an Artificial Satellite’,J. Res. NBS 70B;Math. Math. Phys. 1, 1–16.

    Google Scholar 

  • Vinti, J. P.: 1966b,Mathematische Methoden der Himmelsmechanik und Astrodynamik (ed. by E. Steifel), Bibliographisches Institut, Mannheim, Germany, pp. 97–111.

    Google Scholar 

  • Whittaker, E. T.: 1944,Analytical Dynamics, 4th ed., Dover Publications, New York.

    Google Scholar 

  • Whittaker, E. T. and Watson, G. N.: 1952,Modern Analysis, 4th ed., Camb. Univ. Press., Cambridge, England.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

O'Mathuna, D. Satellite prediction formulae for Vinti's model. Celestial Mechanics 1, 467–478 (1970). https://doi.org/10.1007/BF01231144

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01231144

Keywords

Navigation