Accurate identification of meteoroid streams is crucial for understanding their origins and evolution, especially for missions like ESA's LUMIO that rely on meteor shower observations.
This study assesses the performance of the HDBSCAN unsupervised clustering algorithm in identifying meteoroid streams and compares it with the traditional CAMS look-up table method.
Using three different feature vectors, HDBSCAN successfully identifies meteoroid streams, with 39 streams confirmed using the GEO vector and 30 using the ORBIT vector.
HDBSCAN, while requiring careful parameter selection, outperformed the CAMS method in statistical coherence, showing potential as an effective alternative for meteoroid stream identification.