From a Lagrangian approach for the development of the relative motion equations viewed as a nonlinear Hill’s problem, it is shown that the influence of a spherical primary mass takes the form of a third-body-like disturbing function expressed relative to the origin of Hill’s rotating frame. The resulting Lagrangian and corresponding equations of motion are compact and provide an easily obtainable representation of the nonlinear contributions to the motion to an arbitrary order using recursion relations. The relative motion equations are expanded through third-order in the local Hill’s coordinates and a correspondingly accurate successive approximations solution is developed to describe nonlinear periodic motions in Hill’s frame.


    Access

    Check access

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    A Third-Order Analytical Solution for Relative Motion with a Circular Reference Orbit


    Additional title:

    J of Astronaut Sci


    Contributors:

    Published in:

    Publication date :

    2003-03-01


    Size :

    12 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English




    A Third-Order Analytical Solution for Relative Motion with a Circular Reference Orbit

    Richardson, D. L. / Mitchell, J. W. | Online Contents | 2003



    A Third-Order Analytical Solution for Relative Motion With a Circular Reference Orbit (AAS 02-147)

    Richardson, D. L. / Mitchell, J. W. / American Institute of Aeronautics and Astronautics et al. | British Library Conference Proceedings | 2002