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A graph neural network approach to star identification for navigation without GPS, tested on real nighttime terrestrial data rather than only synthetic or space imagery. The main ML contributions are a more realistic noise model for training, Fourier-transformed edge features, and RANSAC-based alignment. The reported gains are in identification accuracy and solve rate, with attitude accuracy and runtime roughly unchanged, so readers should check how the results hold up under the paper's full evaluation and the released code and data.
SIGNN++: Robust Graph Neural Star Identification on Earth
arXiv:2610.30186v1 Announce Type: cross Abstract: We present SIGNN++, a learning-based star identification (SID) framework for celestial navigation in GNSS-denied nighttime environments. Although researchers have developed learning-based SID methods to improve robustness to observation noise, prior evaluations have focused mainly on synthetic or non-terrestrial environments, leaving their reliability under real terrestrial conditions unclear. To address these limitations, SIGNN++ extends SIGNN, a graph neural network-based SID method, with three components: a more realistic noise model for training data, Fourier Transform (FT) of angular-distance edge features, and RANSAC-based Perspective Star Alignment for identification and attitude refinement. The results show that SIGNN++ is more robust to terrestrial observation disturbances and achieves higher star identification accuracy and solved rates than the original SIGNN and publicly available SID baselines, while maintaining comparable attitude accuracy and practical computation time for continuous operation. The implementation code of SIGNN++ and datasets will be available at https://signnpp.github.io/signnpp/.
Abstract:We present SIGNN++, a learning-based star identification (SID) framework for celestial navigation in GNSS-denied nighttime environments. Although researchers have developed learning-based SID methods to improve robustness to observation noise, prior evaluations have focused mainly on synthetic or non-terrestrial environments, leaving their reliability under real terrestrial conditions unclear. To address these limitations, SIGNN++ extends SIGNN, a graph neural network-based SID method, with three components: a more realistic noise model for training data, Fourier Transform (FT) of angular-distance edge features, and RANSAC-based Perspective Star Alignment for identification and attitude refinement. The results show that SIGNN++ is more robust to terrestrial observation disturbances and achieves higher star identification accuracy and solved rates than the original SIGNN and publicly available SID baselines, while maintaining comparable attitude accuracy and practical computation time for continuous operation. The implementation code of SIGNN++ and datasets will be available at this https URL.
Instrumentation and Methods for Astrophysics (astro-ph.IM); Machine Learning (cs.LG)
arXiv:2610.30186 [astro-ph.IM]
(or arXiv:2610.30186v1 [astro-ph.IM] for this version)
https://doi.org/10.48550/arXiv.2610.30186 Focus to learn more arXiv-issued DOI via DataCite (pending registration)
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