Me. Hough, INTEGRAL SURFACES WITH SPACE-TIME COORDINATES, IN THE GRAVITATIONAL-FIELD OF A ROTATING SYSTEM, Celestial mechanics & dynamical astronomy, 62(3), 1995, pp. 263-287
A new integration theory is formulated for dynamical systems with two
degrees of freedom, in the gravitational field of a rotating system. F
our integrals of motion may be determined from complete solutions of a
system of three first-order, partial differential equations in three
independent variables. The solutions of this system define two integra
l surfaces with space-time coordinates. These surfaces represent two i
ndependent solutions of a second-order kinematic system to which the o
riginal fourth-order system has been reduced. An integral curve may be
represented as the locus of intersection points of the integral surfa
ces. The new theory is the theoretical basis for a method of analytic
continuation of periodic orbits of the circular restricted problem.