Application of machine learning to discover dynamical structures in 4D Poincaré maps in the circular restricted three-body problem

IF 2.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Kevin M. Trigg, Daniel J. Broyles, Robert A. Bettinger, Tyler J. Kapolka
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Abstract

The spatial Circular Restricted Three-Body Problem (CR3BP) produces complex orbital dynamics that are difficult to classify at scale using traditional, manual Poincaré map analysis. A Poincaré map simplifies continuous orbital motion by recording the points where a trajectory intersects a chosen surface in phase space, converting a continuous path into a discrete set of crossings that reveal underlying topological structure. These crossings make it easier to characterize trajectory behavior, but interpreting them visually becomes impractical for large datasets and as Poincaré maps evolve from two into four dimensions. To address this challenge, an unsupervised clustering pipeline for discovering dynamical structures in four-dimensional (4D) Poincaré maps is introduced. Each trajectory’s Poincaré crossings are transformed into a compact feature representation capturing geometric dispersion, statistical, and frequency-based characteristics, enabling density-based clustering without prior labels. The method is evaluated across multiple Jacobi constants to assess robustness, and expanded to investigate chaining dynamical structures to find similar structures across different Jacobi constants. The results demonstrate that feature-based clustering can recover meaningful dynamical structures in high-dimensional trajectory data.

机器学习在圆受限三体问题中四维庞卡罗图动态结构发现中的应用
空间圆形受限三体问题(CR3BP)产生复杂的轨道动力学,难以使用传统的手工庞卡罗地图分析在尺度上进行分类。庞加莱图通过记录轨迹在相空间中与选定表面相交的点来简化连续的轨道运动,将连续的路径转换成一组离散的交叉点,从而揭示潜在的拓扑结构。这些交叉点可以更容易地描述轨迹行为,但对于大型数据集和庞加莱图从二维发展到四维来说,从视觉上解释它们变得不切实际。为了解决这一挑战,引入了一种无监督聚类管道,用于发现四维(4D) poincarcar地图中的动态结构。每个轨迹的poincar交叉点被转换成一个紧凑的特征表示,捕获几何分散、统计和基于频率的特征,从而实现基于密度的聚类,而无需事先标记。该方法跨越多个雅可比常数进行评估,以评估鲁棒性,并扩展到研究链式动力结构,以寻找跨越不同雅可比常数的相似结构。结果表明,基于特征的聚类可以恢复高维轨迹数据中有意义的动态结构。
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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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