Abstract
In this paper the fixed energy surfaces for the two-body problem for parabolic and, in particular, hyperbolic motion are completely, determined by utilizing an earlier work of J. Moser. The characterization of these fixed energy manifolds yields the explicit solutions to the above problems in an elementary way for arbitrary dimensions.
Similar content being viewed by others
References
Hamilton, Sir William R.: 1845–47,The Hodograph or a New Method of Expressing in Symbolic Language the Newtonian Law of Attraction, Proc. Royal Irish Acad. Vol.III, pp. 344–353 (see December 1846).
Möbius, A. F.: 1843,Die Elemente der Mechanik des Himmels, Weidmannsche Buchandlung, Leipzig, pp. 28–59, (Gesammelte Werke, Vol. IV., Verlag von S. Hirzel, 1887).
Moser, J.: 1970,Comm. Pure Appl. Math. 23, 609–636.
Osipov, Yu.: 1972,Geometrical Interpretation of Kepler's Problem., Russian Mathematical Surveys,27, Part I, p. 161.
Siegel, C. L. and Moser, J.: 1971,Lectures, on Celestial Mechanics, Springer-Verlag, New York, pp. 39–40.
Stiefel, E. L. and Scheifele, G.: 1971,Linear and Regular Celestial Mechanics, Springer-Verlag, N.Y.
Sun, F. T.: 1966,A Special Hodograph for Orbital Motion, 2nd International Symposium on Rockets and Astronautics, Tokyo, May 1960, Proc. Yokendo Bunkyo-Ku, Tokyo (in particular, see p. 170).
Sun, F. T.: 1969,On the use of Hodographic Mapping in Trajectory Analysis, N.A.S.A., PM-82.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Belbruno, E.A. Two-body motion under the inverse square central force and equivalent geodesic flows. Celestial Mechanics 15, 467–476 (1977). https://doi.org/10.1007/BF01228612
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF01228612