Fuel Optimal Maneuver of Passive and Periodic Circular-Like Satellite Formation: Legendre Pseudospectral Approach

2013 ◽  
Vol 389 ◽  
pp. 834-840
Author(s):  
Guang Yan Xu ◽  
Xiao Ying Wang

In this paper, an effective method was proposed to formulate and solve a fuel-optimal satellites maneuver control problem using a continuous low-thrust system. The design of the bounded desired final satellite formation is a passive and periodic circular-like formation at critical inclination underperturbation, which adjusts to long-term flying formation. The nonlinear optimal control problem is converted into a nonlinear programming problem by the application of the Legendre pseudospectral method. Due to the design includes the free final time and the precise final condition constraint, fuel-optimal maneuver is more reasonable, thereby it will achieve the minimum fuel consumption.

2014 ◽  
Vol 926-930 ◽  
pp. 3688-3691
Author(s):  
Jian Wei Shi ◽  
Yuan Wen Cai ◽  
Xiao Chen Xing

Aim to the path programme problem of satellite formation reconfiguration under low thrust, optimization is simulated based on Gauss Pseudospectral Method (GPM). The simulation result demonstrates that the GPM can effectively solve the the path optimization problem.


2021 ◽  
Vol 133 (3) ◽  
Author(s):  
Marilena Di Carlo ◽  
Simão da Graça Marto ◽  
Massimiliano Vasile

AbstractThis paper presents a collection of analytical formulae that can be used in the long-term propagation of the motion of a spacecraft subject to low-thrust acceleration and orbital perturbations. The paper considers accelerations due to: a low-thrust profile following an inverse square law, gravity perturbations due to the central body gravity field and the third-body gravitational perturbation. The analytical formulae are expressed in terms of non-singular equinoctial elements. The formulae for the third-body gravitational perturbation have been obtained starting from equations for the third-body potential already available in the literature. However, the final analytical formulae for the variation of the equinoctial orbital elements are a novel derivation. The results are validated, for different orbital regimes, using high-precision numerical orbit propagators.


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