Abstract
This paper presents two peculiar geometrical structures in the configuration space of the classical Kepler problem: the circularU-graph and the circularS-graph. TheS-graph shows up a configuration space counterpart of the well-known velocity space hodograph. Several interesting results are brought out, such as a peculiar description of the mechanical energy. An extension to the three-dimensional space, through theU-sphere and theS-sphere, characterizes the regular Kepler orbits by means of the north pole of the associatedS-sphere. The Minkowskian parameterization introduced in [1] is easily recovered and is shown to fit naturally in theS-sphere description of the Kepler problem.
Similar content being viewed by others
References
Cariñena, J.F., López, C., Del Olmo M.A., Santander M., Conformal Geometry of the Kepler Orbit Space, Celest. Mech. and Dynam. Astron. 52(1991), 307–343.
Vivarelli, M.D., The KS-Transformation Revisited, Meccanica 29(1994), 15–26.
Vivarelli, M.D., The Kepler Problem: A Unifying View, Celest. Mech. and Dynam. Astron. 60(1994), 291–305.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Vivarelli, M.D. A Configuration Counterpart of the Kepler Problem Hodograph. Celestial Mechanics and Dynamical Astronomy 68, 305–311 (1997). https://doi.org/10.1023/A:1008223102613
Issue Date:
DOI: https://doi.org/10.1023/A:1008223102613