🤖 AI Summary
This study addresses the limitations of traditional Gaussian orbit determination methods, which rely on the two-body assumption and fail under the strong three-body perturbations and extreme uncertainties characteristic of cislunar space. To overcome this challenge, the authors propose a hybrid particle Gaussian mixture filtering framework—termed PGM-I and PGM-II—that is, to the best of the authors’ knowledge, the first application of such an architecture to cislunar orbit determination. The approach constructs a purely recursive probabilistic model that effectively integrates ground-based angle-only observations, thereby handling the pronounced nonlinearity and non-Gaussian uncertainty inherent in the problem. Experimental results demonstrate that the proposed method significantly enhances both accuracy and robustness in representative cislunar orbit scenarios, achieving reliable probabilistic orbit tracking using only angular measurements.
📝 Abstract
Gauss's method of orbit determination (OD) and its variants are among the most popular initial state estimation techniques for astronomers and engineers alike. However, owing to its assumptions regarding the two-body problem, Gauss's method is inapplicable in the cislunar domain, where three body effects dominate. We introduce a hybrid Particle Gaussian Mixture filtering method, a purely recursive probabilistic orbit determination framework based on a combination of the Markov Chain Monte Carlo based Particle Gaussian Mixture-II (PGM-II) and Particle Gaussian Mixture-I (PGM-I) filters. This method enables us to fuse probabilistic information with angles-only observations from terrestrial telescopes for short and long-term cislunar target tracking. We demonstrate this technique on an important cislunar orbit regime.