Abstract

Spacecraft need to be able to reliably slew quickly and rather than simply commanding a final angle, a trajectory calculated and known throughout a maneuver is preferred. A fully solved trajectory allows for control based off comparing current attitude to a time varying desired attitude, allowing for much better use of control effort and command over slew orientation. This manuscript introduces slew trajectories using sinusoidal functions compared to optimal trajectories using Pontryagin’s method. Use of Pontryagin’s method yields approximately 1.5% lower control effort compared to sinusoidal trajectories. Analysis of the simulated system response demonstrates that correct understanding of the effect of cross-coupling is necessary to avoid unwarranted control costs. Additionally, a combination of feedforward with proportional derivative control generates a system response with 3% reduction in control cost compared to a Feedforward with proportional integral derivative control architecture. Use of a calculated trajectory is shown to reduce control cost by five orders of magnitude and allows for raising of gains by an order of magnitude. When control gains are raised, an eight orders of magnitude lower error is achieved in the slew direction, and rather than an increase in control cost, a decrease by 11.7% is observed. This manuscript concludes that Pontryagin’s method for generating slew trajectories outperforms the use of sinusoidal trajectories and trajectory generation schemes are essential for efficient spacecraft maneuvering.

Highlights

  • IntroductionThe. James Webb Space telescope (JWST) will study the formation of stars, galaxies, and planets

  • To see the first stars and galaxies of the early universe, James Webb Space telescope (JWST) must look deep into space, necessitating a need for fine pointing accuracy, one of the reasons JWST is positioned so far away from Earth and the perturbations of the atmosphere

  • Due to the incredible distance between the JWST and potential imaging targets, pointing errors of mere arcseconds can lead to the telescope field of view not including the intended target, and any spacecraft jitter results in blurry, unusable images

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Summary

Introduction

The. James Webb Space telescope (JWST) will study the formation of stars, galaxies, and planets. To see the first stars and galaxies of the early universe, JWST must look deep into space, necessitating a need for fine pointing accuracy, one of the reasons JWST is positioned so far away from Earth and the perturbations of the atmosphere. Due to the incredible distance between the JWST and potential imaging targets, pointing errors of mere arcseconds can lead to the telescope field of view not including the intended target, and any spacecraft jitter results in blurry, unusable images. Lower control costs result in “cheaper” maneuvers, which can allow for less expensive spacecraft launch, due to mass savings, more possible maneuvers over the spacecraft lifetime due to energy savings, or greater error tolerances and recovery capabilities

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