Abstract
A complex of standard programmes has been developed for computing nearly parabolic orbits. The true anomaly is related to the time using Herrick’s formulae. Perturbations are calculated by Encke’s method.
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References
Dubyago, A. D.: 1949, Opredelenie Orbit, Moscow, p. 293
Herrick, C. E.: 1960, Details of Computational Methods: Space Trajectories, p. 135.
Kazimirchak-Polonskaya, E. I.: 1967, Trudy Inst. Teor. Astron. 12, 24.
Nikonova, L. E.: 1968, Trudy Astron. Obs. Kazan No. 35, 169.
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© 1972 IAU
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Nikonova, L.E., Bokhan, N.A. (1972). Standardization of the Calculation of Nearly Parabolic Cometary Orbits. In: Chebotarev, G.A., Kazimirchak-Polonskaya, E.I., Marsden, B.G. (eds) The Motion, Evolution of Orbits, and Origin of Comets. International Astronomical Union / Union Astronomique Internationale, vol 45. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2873-8_24
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DOI: https://doi.org/10.1007/978-94-010-2873-8_24
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