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Autonomous Angles-Only Navigation for Spacecraft Swarms around Planetary Bodies

机译:仅自动角度 - 仅航天器围绕行星体群的航行

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This paper presents and demonstrates an algorithmic framework for autonomous navigation of spacecraft swarms around planetary bodies, using angles-only measurements from onboard cameras. Angles-only methods are compelling as they reduce reliance on external measurement sources. However, prior demonstrations have faced limitations, including 1) inability to treat more than one observer and target in a swarm, 2) lack of autonomy and reliance on external state information, and 3) treatment of only Earth-orbit scenarios. The new Absolute and Relative Trajectory Measurement System (ARTMS) overcomes these challenges and consists of three core modules leveraging novel algorithms: Image Processing, which tracks and identifies targets in images and computes their bearing angles; Batch Orbit Determination, which computes a swarm state initialization from angles-only measurements; and Sequential Orbit Determination, which uses an unscented Kalman filter to refine the swarm state estimate, seamlessly fusing measurements from multiple observers to achieve the autonomy, robustness and distribution needed for deep space navigation. Theoretical performance of ARTMS is investigated through a quantitative observability analysis of multi-observer angles-only navigation in Mars orbit. For swarms of at least 3 spacecraft and at least 2 observers, the complete swarm state is observable. After two orbits, the absolute orbit is estimated to within 1 km, target ranges are estimated to within 0.5%, and other relative state components are estimated to 0.02% of target range. Clock offsets are estimated to within 0.05s. These accuracies are validated with camera-in-the-loop simulations of a four-spacecraft swarm taking distributed measurements in an eccentric Mars orbit. ARTMS displays robust navigation across a variety of formations and under challenging conditions, and achieves the necessary performance to support the proposed objectives.
机译:本文介绍并展示了航天器围绕行星体群的自主导航的算法框架,使用船上摄像机的角度测量。只有角度的方法是引人注目的,因为它们减少了对外部测量来源的依赖。然而,现有示范面临局面,包括1)无法治疗一个以上的观察者和目标,2)缺乏自主性和对外部状态信息的依赖,以及仅处理地球轨道场景。新的绝对和相对轨迹测量系统(ARTMS)克服了这些挑战,包括利用新算法的三个核心模块:图像处理,其追踪和识别图像中的目标并计算其轴承角度;批量轨道确定,从唯一的角度测量计算群状态初始化;和顺序轨道确定,它使用Unscented Kalman滤波器来改进群体状态估计,从多个观察者无缝融合测量,以实现深度空间导航所需的自主,鲁棒性和分布。通过MARS轨道中的多观察角度的定量可观察性分析来研究ARTMS的理论性能。对于至少3个航天器和至少2个观察者的群体,可以观察到完整的群状态。在两个轨道之后,绝对轨道估计在1公里内,估计目标范围在0.5%以内,并且其他相对状态分量估计为0.02%的目标范围。时钟偏移量估计到0.05s。这些准确性验证了使用四个航天器群的环路模拟,以偏心火星轨道中的分布测量。 ARTMS在各种地层和在挑战条件下显示强大的导航,并实现了支持拟议目标的必要性能。

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