“…Let (g, ξ ) ∈ SE(3) × R 6 denote the states (configuration and velocities) of the spacecraft. Given the asteroid trajectory generated by (8) and (13), the desired states of the spacecraft are g 0d = g 0 (h f ) and ξ 0d = Ad (h f ) −1 ξ 0 for t ≥ t 0 , (38) and the configuration error between the spacecraft and the asteroid is…”
Section: A Setting Up the Relative Configurationmentioning
confidence: 99%
“…Given η = [ T β T ] T ∈ R 6 , the function G(η) can be expressed as a block-triangular matrix, as follows [38]:…”
Section: Remark 1 the Logarithm Map Logm:se(3) → Sementioning
confidence: 99%
“…The desired state trajectory of the spacecraft required to maintain the formation is given by the desired configuration g 0 and its time derivative, which gives the desired velocities ξ 0 = Ad (h f ) −1 ξ 0 as in (38). Let us denote the desired state trajectory for time t ≥ t 0 by the desired position vector in the inertial frame b 0 (t), the desired attitude R 0 (t), and the desired translational and angular velocity in the body frame, ν 0 (t) and 0 (t).…”
Section: B Trajectory Tracking Errorsmentioning
confidence: 99%
“…The feedback system given by (43) and (49) and the control scheme in (50) globally stabilizes (η,ξ ) = (0, 0) ∈ R 6 × R 6 and therefore tracks the trajectory (g, ξ ) = (g 0 , ξ 0 ) given by (38) in finite time. Moreover, the domain of attraction of this trajectory is almost global over the state space…”
Section: Finite-time Control Scheme For Body-fixed Spacecraft Hovementioning
A finite-time control scheme for autonomous body-fixed hovering of a rigid spacecraft over a tumbling asteroid is presented. The relative configuration between the spacecraft and asteroid is described in terms of exponential coordinates on the Lie group SE(3), which is the configuration space for the spacecraft. With a Lyapunov stability analysis, the finite-time convergence of the proposed control scheme for the closed-loop system is proved. Numerical simulations validate the performance of the proposed control scheme.
“…Let (g, ξ ) ∈ SE(3) × R 6 denote the states (configuration and velocities) of the spacecraft. Given the asteroid trajectory generated by (8) and (13), the desired states of the spacecraft are g 0d = g 0 (h f ) and ξ 0d = Ad (h f ) −1 ξ 0 for t ≥ t 0 , (38) and the configuration error between the spacecraft and the asteroid is…”
Section: A Setting Up the Relative Configurationmentioning
confidence: 99%
“…Given η = [ T β T ] T ∈ R 6 , the function G(η) can be expressed as a block-triangular matrix, as follows [38]:…”
Section: Remark 1 the Logarithm Map Logm:se(3) → Sementioning
confidence: 99%
“…The desired state trajectory of the spacecraft required to maintain the formation is given by the desired configuration g 0 and its time derivative, which gives the desired velocities ξ 0 = Ad (h f ) −1 ξ 0 as in (38). Let us denote the desired state trajectory for time t ≥ t 0 by the desired position vector in the inertial frame b 0 (t), the desired attitude R 0 (t), and the desired translational and angular velocity in the body frame, ν 0 (t) and 0 (t).…”
Section: B Trajectory Tracking Errorsmentioning
confidence: 99%
“…The feedback system given by (43) and (49) and the control scheme in (50) globally stabilizes (η,ξ ) = (0, 0) ∈ R 6 × R 6 and therefore tracks the trajectory (g, ξ ) = (g 0 , ξ 0 ) given by (38) in finite time. Moreover, the domain of attraction of this trajectory is almost global over the state space…”
Section: Finite-time Control Scheme For Body-fixed Spacecraft Hovementioning
A finite-time control scheme for autonomous body-fixed hovering of a rigid spacecraft over a tumbling asteroid is presented. The relative configuration between the spacecraft and asteroid is described in terms of exponential coordinates on the Lie group SE(3), which is the configuration space for the spacecraft. With a Lyapunov stability analysis, the finite-time convergence of the proposed control scheme for the closed-loop system is proved. Numerical simulations validate the performance of the proposed control scheme.
“…In order to describe the 6-DOF relative-motion in a united framework and facilitate the controller synthesis work, constructing coupled dynamics by the relative position and attitude described on the Lie group SE (3) has been an effective tool and received increasing attention in [2], [10][11][12][13][14][15]. In [2], a sliding mode control scheme on the coupled dynamics on SE(3) was presented to achieve the desired formation with respect to the virtual leader whose trajectory was computed offline.…”
This paper presents an approach for designing angular and linear velocity observers for rigid bodies using two inertial vectors and one landmark measurements directly. Compared with the classical velocity estimation algorithms, the proposed observer does not need to reconstruct the pose information from measurements nor be coupled with velocity sensors. The linear‐time varying dynamics of the estimation error equation are analyzed, rigorously showing the uniform local exponential stability of the observer. Simulations are conducted to illustrate the significant performance of the proposed method.
scite is a Brooklyn-based organization that helps researchers better discover and understand research articles through Smart Citations–citations that display the context of the citation and describe whether the article provides supporting or contrasting evidence. scite is used by students and researchers from around the world and is funded in part by the National Science Foundation and the National Institute on Drug Abuse of the National Institutes of Health.