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Identifying Cislunar Orbital Families via Machine Learning on Light Curves

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Abstract

Current methods of performing Initial Orbit Determination (IOD) in near-earth orbital regions cannot be directly extended to cislunar space due to changes in gravitational models that must be utilized. For the case of cislunar orbits, the Moon’s gravitational influence necessitates that orbital motions be described by three-body dynamics. Three-body dynamics produce orbits that are generally not elliptical, fixed to an orbital plane, or geometrically simple. This change in assumptions that can be made complicates the task of performing IOD and has led to the investigation of alternative methods and features to classify cislunar orbit parameters. In this paper, we explore the potential of utilizing Machine Learning (ML) algorithms to constrain potential IOD search spaces to specific cislunar families. We accomplish this by training the ML classifier to predict cislunar family from a light curve. To generate training data for this ML effort, we introduce a novel simulation pipeline that produces radiometrically validated light curves using the Digital Imaging and Remote Sensing Image Generation (DIRSIG™) engine. This pipeline ingests various parameters, including: initial Circular Restricted Three-Body Problem (CR3BP) state vectors, satellite material properties, telescope optical properties, and satellite 3D models. The pipeline produces light curves capturing the influence of these factors on the observed visual magnitude signature as a function of elapsed time and phase angle. This pipeline was utilized to produce approximately 3500 light curves of various cislunar orbital families as captured from the perspective of two observing locations: the spaced-based Earth-Moon L1 point, and a Lunar surface based point. These light curves were used as training datasets for neural network models to perform classification of cislunar family via input time-series vectors consisting of two features: visual magnitude and phase angle. Our machine learning technique first uses a warping technique to construct constant sized observational input of the light curves into a multi-layer perceptron, the architecture of which was chosen by a search over a large landscape of possibilities optimizing for validation prediction accuracy. The selected model was then trained on various scenarios of input data, again doing a search over several available hyper-parameters. It was found that the trained models were able to achieve test data-set accuracy of 93.4% for light curves captured from the face of the moon, and 87.5% when combined with light curves captured from the space-based L1 point.

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Acknowledgements

We would like to thank GTRI’s Independent Research and Development (IRAD) funds for supporting this work. On behalf of all authors, the corresponding author states that there is no conflict of interest.

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Correspondence to Gregory P. Badura.

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Appendix

Appendix

Table 6 gives an overview of the initial state vectors that were used to generate light curves for this study.

Table 6 Initial dimensionless state vectors of the cislunar satellite targets that were used to generate light curves in this study for both a lunar-based telescope and a space-based telescope at the Earth-Moon L1 point

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Badura, G.P., DeBlasio, D., Najera, A. et al. Identifying Cislunar Orbital Families via Machine Learning on Light Curves. J Astronaut Sci 71, 27 (2024). https://doi.org/10.1007/s40295-024-00447-6

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