Kevin M. Trigg, Daniel J. Broyles, Robert A. Bettinger, Tyler J. Kapolka
{"title":"Application of machine learning to discover dynamical structures in 4D Poincaré maps in the circular restricted three-body problem","authors":"Kevin M. Trigg, Daniel J. Broyles, Robert A. Bettinger, Tyler J. Kapolka","doi":"10.1007/s10509-026-04638-5","DOIUrl":null,"url":null,"abstract":"<div><p>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.</p></div>","PeriodicalId":8644,"journal":{"name":"Astrophysics and Space Science","volume":"371 9","pages":""},"PeriodicalIF":2.1000,"publicationDate":"2026-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s10509-026-04638-5.pdf","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astrophysics and Space Science","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10509-026-04638-5","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
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.
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.