Abstract

The integrated 6-DOF orbit-attitude dynamical modeling and control have shown great importance in various missions, for example, formation flying and proximity operations. The integrated approach yields better performances than the separate one in terms of accuracy, efficiency, and agility. One challenge in the integrated approach is to find a unified representation for the 6-DOF motion with configuration space SE(3). Recently, exponential coordinates of SE(3) have been used in dynamics and control of the 6-DOF motion, however, only on the kinematical level. In this paper, we will improve the current method by adopting exponential coordinates on the dynamical level, by giving the relation between the second-order derivative of exponential coordinates and spacecraft’s accelerations. In this way, the 6-DOF motion in terms of exponential coordinates can be written as a second-order system with a quite compact form, to which a broader range of control theories, such as higher-order sliding modes, can be applied. For a demonstration purpose, a simple asymptotic tracking control law with almost global convergence is designed. Finally, the integrated modeling and control are applied to the body-fixed hovering over an asteroid and verified by a simulation, in which absolute motions of the spacecraft and asteroid are simulated separately.

Highlights

  • The orbit and attitude motions are kinematically coupled in spacecraft relative motions [1, 7] and are dynamically coupled due to effects of external forces and torques, such as the gravitational orbitattitude coupling in close proximity of minor celestial bodies [18,19,20,21] and the orbit-attitude coupling of high area-to-mass ratio (HAMR) objects caused by the solar radiation pressure (SRP) [22, 23]

  • The integrated 6-DOF orbit-attitude dynamical modeling and controller design for the relative motion of spacecraft with respect to a reference body have been studied in the framework of geometric mechanics in the present paper

  • The configuration and velocity of the relative motion have been represented by the Lie group SE(3) and its exponential coordinates

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Summary

Introduction

The integrated 6-DOF orbit-attitude dynamical modeling and control of spacecraft have shown great importance in various space missions, such as formation flying [1,2,3,4,5,6,7], proximity operations [8,9,10,11,12,13,14], and proximity operations about minor celestial bodies [15,16,17]. Exponential coordinates of Lie group SE(3) have been used as a unified representation of the 6-DOF orbit-attitude (rigid body) motion in spacecraft formation flying and asteroid hovering [6, 9, 14,15,16,17]. Exponential coordinates of SE(3) used by Lee et al [6, 15, 16] have provided a good unified representation for the 6-DOF motion with several advantages: having a vector form, having no constraint between elements, being convenient for controller design, and achieving almost global convergence in the controller. Based on the second-order system in terms of exponential coordinates of SE(3), a simple asymptotic tracking control law with almost global convergence is designed for a demonstration purpose Both the integrated dynamical modeling and control law are applied to body-fixed orbitattitude hovering over an asteroid

Integrated Modeling of 6-DOF Relative Dynamics
Tracking Error Modeling and Control Law Design
Body-Fixed Orbit-Attitude Hovering over an Asteroid
Conclusions
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