Abstract
Szebehely's partial differential equation for the force functionU=U(x,y) which gives rise to a given family of planar orbitsf(x,y)=Constant is generalized to account for velocity-dependent potentials V*=V*(x,y,\(\dot x,\dot y\)). The new partial differential equation is quasi-linear and of the first order. An example is given and a comparison is made of the two equations.
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References
Broucke, R. and Lass, H.: 1977,Celes. Mech. 16, 215.
Goldstein, H.: 1970,Classical Mechanics, Chapter 1, p. 19, Addison-Wesley Publ. Co. Inc.
Molnar, S.: 1981,Celes. Mech. 25, 79.
Pars, L. A.: 1965,A Treatise on Analytical Dynamics, Chapter VI, p. 82, Heinemann, London.
Szebehely, V.: 1974, ‘On the Determination of the Potential by Satellite Observations’, in E. Proverbio (ed.),Proceedings of the International Meeting on Earth's Rotations by Satellite Observations, University of Cagliari, Bologna, Italy.
Szebehely V. and Broucke, R.: 1981,Celes. Mech. 24, 23.
Whittaker, E. T.: 1937,Analytical Dynamics of Particles and Rigid Bodies, Chapter IV, p. 95, Cambridge Univ. Press.
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Bozis, G. Generalization of Szebehely's equation. Celestial Mechanics 29, 329–334 (1983). https://doi.org/10.1007/BF01228527
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DOI: https://doi.org/10.1007/BF01228527