Attitude stability of artificial satellites subject to gravity gradient torque
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Data
2009-08-01
Autores
de Moraes, Rodolpho Vilhena [UNESP]
Santos Cabette, Regina Elaine [UNESP]
Zanardi, Maria Cecilia [UNESP]
Stuchi, Teresinha J.
Formiga, Jorge Kennety
Título da Revista
ISSN da Revista
Título de Volume
Editor
Springer
Resumo
The stability of the rotational motion of artificial satellites is analyzed considering perturbations due to the gravity gradient torque, using a canonical formulation, and Andoyer's variables to describe the rotational motion. The stability criteria employed requires the reduction of the Hamiltonian to a normal form around the stable equilibrium points. These points are determined through a numerical study of the Hamilton's equations of motion and linear study of their stability. Subsequently a canonical linear transformation is used to diagonalize the matrix associated to the linear part of the system resulting in a normalized quadratic Hamiltonian. A semi-analytic process of normalization based on Lie-Hori algorithm is applied to obtain the Hamiltonian normalized up to the fourth order. Lyapunov stability of the equilibrium point is performed using Kovalev and Savchenko's theorem. This semi-analytical approach was applied considering some data sets of hypothetical satellites, and only a few cases of stable motion were observed. This work can directly be useful for the satellite maintenance under the attitude stability requirements scenario.
Descrição
Palavras-chave
Rotational motion of artificial satellites, Non linear stability, Normalization
Como citar
Celestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 104, n. 4, p. 337-353, 2009.