AstroSLAM: Autonomous monocular navigation in the vicinity of a celestial small body—Theory and experiments

Mehregan Dor, Travis Driver, Kenneth Getzandanner, Panagiotis Tsiotras
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Abstract

We propose AstroSLAM, a standalone vision-based solution for autonomous online navigation around an unknown celestial target small body. AstroSLAM is predicated on the formulation of the SLAM problem as an incrementally growing factor graph, facilitated by the use of the GTSAM library and the iSAM2 engine. By combining sensor fusion with orbital motion priors, we achieve improved performance over a baseline SLAM solution and outperform state-of-the-art methods predicated on pre-integrated inertial measurement unit factors. We incorporate orbital motion constraints into the factor graph by devising a novel relative dynamics—RelDyn—factor, which links the relative pose of the spacecraft to the problem of predicting trajectories stemming from the motion of the spacecraft in the vicinity of the small body. We demonstrate AstroSLAM’s performance and compare against the state-of-the-art methods using both real legacy mission imagery and trajectory data courtesy of NASA’s Planetary Data System, as well as real in-lab imagery data produced on a 3 degree-of-freedom spacecraft simulator test-bed.
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AstroSLAM:小天体附近的自主单目导航--理论与实验
我们提出的 AstroSLAM 是一种基于视觉的独立解决方案,用于围绕未知天体目标小体进行自主在线导航。AstroSLAM 的前提是将 SLAM 问题表述为一个增量增长的因子图,而 GTSAM 库和 iSAM2 引擎的使用则为这一表述提供了便利。通过将传感器融合与轨道运动先验相结合,我们实现了比基线 SLAM 解决方案更高的性能,并超越了基于预集成惯性测量单元因子的最先进方法。我们通过设计一种新颖的相对动力学因子(RelDyn-factor)将轨道运动约束条件纳入因子图,该因子将航天器的相对姿态与预测航天器在小天体附近的运动轨迹问题联系起来。我们展示了 AstroSLAM 的性能,并使用美国国家航空航天局行星数据系统提供的真实遗留飞行任务图像和轨迹数据,以及在 3 自由度航天器模拟器测试平台上生成的真实实验室内图像数据,与最先进的方法进行了比较。
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