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Probabilistic Tracklet Clustering and Initial Orbit Determination

  • Beijing Institute of Technology
  • University of New South Wales
  • Beijing Aerospace Flight Control Center

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

Space Situational Awareness (SSA) is critical for monitoring the increasing number of space objects. A key component of SSA is tracklet clustering, which involves integrating fragmented observation data from multiple sensors to construct continuous trajectories. Effective tracklet clustering facilitates object identification and initial orbit determination (IOD), thereby enhancing collision avoidance and space traffic management. The primary challenge in tracklet clustering is managing the vast volume of observation data. Deploying mega-constellations has significantly expanded the number of observable space objects. Traditional approaches struggle to establish accurate correlations within such large datasets, particularly in the case of constellation satellites. Moreover, optical tracklets frequently arise from short observation arcs, leading to significant uncertainty in angular velocity, which further complicates the association of multiple tracklets with a single object. To overcome these challenges, this paper develops a probabilistic tracklet clustering method and a robust IOD method based on clustering. The process begins with an initial association executed via the Boundary Value Problem-Constrained Admissible Region Optimization method (BVP-CAR-Opt). The association probability between two tracklets is assessed through the Mahalanobis distance between the measured and estimated angular-rate information. The tracklet clustering is formulated as an optimization problem. The optimization objective is to maximize the likelihood of the association matrix, which is calculated based on the association probabilities obtained through the BVP-CAR-Opt method. This progress achieves efficient and accurate tracklet clustering by solving the optimal association matrix, avoiding the exhaustive enumeration of all hypotheses. Once the clusters are determined, the weighted hypothetical orbits are generated by the BVP-CAR-Opt according to their corresponding association probabilities. These weighted hypothetical orbits are subsequently utilized in the least squares algorithm to yield the initial orbit. Incorporating weighting factors significantly reduces the relative influence of the assumed orbits on error estimation, thereby ensuring a stable and consistent initial orbit. To evaluate the performance of the developed method, one simulation scenario was employed and compared with Markov clustering techniques. Optical observation data were generated from a LEO space-based sensor. The tracklet clustering was applied to 30 randomly selected space objects from the 18th Space Defense Squadron public catalog. The new approach demonstrates a higher tracklet clustering accuracy compared with Markov clustering, affirming its effectiveness in typical scenarios.

Original languageEnglish
Title of host publication23rd IAA Symposium on Space Debris - Held at the 76th International Astronautical Congress, IAC 2025
PublisherInternational Astronautical Federation, IAF
Pages642-651
Number of pages10
ISBN (Electronic)9798331329273
DOIs
Publication statusPublished - 2025
Event23rd IAA Symposium on Space Debris at the 76th International Astronautical Congress, IAC 2025 - Sydney, Australia
Duration: 29 Sept 20253 Oct 2025

Publication series

NameProceedings of the International Astronautical Congress, IAC
Volume2-F218712
ISSN (Print)0074-1795

Conference

Conference23rd IAA Symposium on Space Debris at the 76th International Astronautical Congress, IAC 2025
Country/TerritoryAustralia
CitySydney
Period29/09/253/10/25

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