用于小卫星视觉姿态传播的恒星陀螺仪设计

S. Rawashdeh, W. C. Danhauer, J. Lumpp
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引用次数: 9

摘要

姿态确定对许多立方体卫星来说是至关重要的。然而,CubeSat的质量、体积和功率限制了设计人员的选择。在这项工作中,我们正在开发一个恒星陀螺仪,以产生三个自由度的航天器相对姿态估计,而不存在与大多数固态陀螺仪方法相关的漂移。恒星陀螺仪是一种基于恒星的姿态传播器,它利用成像仪视场中恒星的相对运动。给出了星探测、通信和姿态传播的算法。将随机样本一致性(RANSAC)方法应用于对应问题,以减轻假阳性和假阴性的恒星检测。本文概述了该方法,描述了该方法中具有挑战性的方面的解决方案的细节,评估了实验结果,并为立方体卫星系统的初步设计提供了组件选择。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Design of a Stellar Gyroscope for visual attitude propagation for small satellites
Attitude Determination is critical for many CubeSat class satellites. However, the mass, volume, and power constraints of the CubeSat form factor limit the options available to designers. In this work, we are developing a Stellar Gyroscope to generate spacecraft relative attitude estimates in three degrees of freedom without the drift associated with most solid state based gyroscope approaches. A Stellar Gyroscope is a star based attitude propagator that uses relative motion of stars in an imager's field of view. Algorithms to perform the star detection, correspondence, and attitude propagation are presented. The Random Sample Consensus (RANSAC) approach is applied to the correspondence problem to mitigate false-positive and false-negative star detections. This paper overviews the approach, describes the details of the solutions for the challenging aspects of the approach, evaluates experimental results, and offers component selection for a preliminary designs for a CubeSat system.
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