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Application of Szebehely’s Inverse Problem to Non-Stationary Dynamical Systems
Published online by Cambridge University Press: 12 April 2016
Abstract
A first-order linear partial differential equation is presented, giving the non-stationary potential functions U=U (x,y,t) which give rise to a given family of evoling planar orbits f(x,y,t) = c in two-dimensional dynamical system. It is shown, that this equation is applied in celestial mechanics of variable mass.
- Type
- Part V General Celestial Mechanics and Stellar Dynamics
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- Copyright © Nova Science Publishers 1993