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Time transformations for relative motion

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Abstract

Several methods of time-transformations are presented to compute the relative motion of two gravitationally non-interacting space vehicles with increased accuracy. These methods are well suited for any eccentricities of the participating space vehicles which may be located at any distance.

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References

  • Nacozy, P. and Szebehely, V.: 1976, The Computation of Relative Motion with Increased Precision, this issue, p. 449.

  • Sundman, K.: 1912,Acta Math.,36, 105.

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  • Szebehely, V.: 1976, Three Theorems on Relative Motion,Celestial Mechanics, to be published.

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Authors and Affiliations

  1. University of Texas Austin, Texas

    V. Szebehely

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  1. V. Szebehely
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Szebehely, V. Time transformations for relative motion. Celestial Mechanics 13, 465–470 (1976). https://doi.org/10.1007/BF01229099

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  • DOI: https://doi.org/10.1007/BF01229099

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