COMPATIBLE POTENTIALS AND ORBITS IN SYNODIC SYSTEMS

Citation
G. Bozis et M. Stavinschi, COMPATIBLE POTENTIALS AND ORBITS IN SYNODIC SYSTEMS, Celestial mechanics & dynamical astronomy, 64(4), 1996, pp. 351-361
Citations number
15
Categorie Soggetti
Astronomy & Astrophysics
ISSN journal
09232958
Volume
64
Issue
4
Year of publication
1996
Pages
351 - 361
Database
ISI
SICI code
0923-2958(1996)64:4<351:CPAOIS>2.0.ZU;2-P
Abstract
For a given family of orbits f(x, y) = c which can be traced by a mat erial point of unit in an inertial frame it is known that all potentia ls V(x, y) giving rise to this family satisfy a homogeneous, linear in V(x, y), second order partial differential equation (Bozis, 1984). Th e present paper offers an analogous equation in a synodic system Oxy, rotating with angular velocity omega. The new equation, which relates the synodic potential function Omega(x, y) = -V(x, y) + 1/2 omega(2)(x (2) + y(2)) to the given family f(x, y) = c, is again of the second o rder in Omega(x, y) but nonlinear. As an application, some simple comp atible pairs of functions Omega(x, y) and f(x, y) are found, for appro priate values of omega, by adequately determining coefficients both in Omega and f.