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Asymptotic theory for thrusting,spinning-up spacecraft maneuvers
Authors:Mohammad A Ayoubi  James M Longuski
Institution:1. Centre for Sports and Exercise Medicine, Barts and the London School of Medicine and Dentistry, Mile End Hospital, London E1 4DG, UK;2. Pathology Group, Institute of Cell and Molecular Science, Barts and the London School of Medicine and Dentistry, Queen Mary, University of London, E1 2ES, UK;1. Georgia Institute of Technology, Atlanta, GA 30332, United States;2. The University of Colorado Boulder, Boulder, CO 80305, United States;1. GISTDA Academy, Geo-Informatics and Space Technology Development Agency, Thailand;2. Space Dynamics Laboratory, Department of Mechanical and Control Engineering, Kyushu Institute of Technology (KIT), Japan;1. Department of Aerospace Engineering, Texas A&M University, 741D H.R. Bright Bldg., College Station, TX 77843-3141, USA;2. Department of Aerospace Engineering, Texas A&M University, 745 H.R. Bright Bldg., College Station, TX 77843-3141, USA
Abstract:We consider the problem of a spacecraft subjected to constant body-fixed forces and moments about all three axes during a spinning-up, thrusting maneuver. In applications, undesired forces and moments can arise due to thruster imbalances and misalignments and to center-of-mass offset. In previous works, approximate analytical solutions have been found for the attitude motion, and for the change in inertial velocity and inertial position. In this paper we find asymptotic and limiting-case expressions which we derive from the analytic solutions, in order to obtain simplified, practical formulas that lend insight into the motion. Specifically, we investigate how the motion evolves (1) as time grows without bound and (2) for geometric cases of the sphere, the thin rod, and the thin plate. Closed-forms or upper-bound limits are provided for angular velocities, Eulerian angles, angular momentum pointing error, transverse and axial velocities, and transverse and axial displacements. Summaries for the asymptotic limits (for zero initial conditions) are provided in tabular form. Results are verified by numerical simulations.
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