Error dependencies in the space-based CNEOS fireball database
Abstract
We evaluate the reliability of CNEOS-derived ephemerides of fireball events given the absence of the underlying data. We analyzed 18 events that have both (i) sufficient satellite information to derive orbits and (ii) ground-based observational counterparts. We quantify the uncertainties on these calibrated events using the orbital similarity criterion . We also examine the velocity components imbalance and identify discriminants that can indicate the accuracy of an event. We identify two groups in the CNEOS database. CNEOS data produces ephemeris determinations with <0.1 for fireballs reported either (i) after late 2017 or (ii) with impact energies above 0.45 kt with 74-78% of events having =0.030.02, while ~11% show <0.008. Our statistical test confirms these two parameters as the only reliable discriminants that, when combined, explain the two accuracy groups. Daylight, z-velocity component, low altitude, long duration, and latitude might also indicate errors, although the limited dataset may obscure correlations. No clear discriminants are identified for more restrictive cut-offs. We provide estimates of orbital uncertainties for calibrated events. The hyperbolic fireball subset in the CNEOS database appears as an outlier in the velocity imbalance test. Our results confirm that the fidelity of CNEOS fireball data improved significantly from 2018, likely due to the deployment of next-generation space sensors, and show a growing number of high-velocity events. Hyperbolic candidates should be interpreted with caution, as their velocities and inclinations likely reflect measurement errors. Accuracy constraints remain limited by the dataset size, as evidenced by the lack of statistically significant dependence on duration, preventing strong conclusions from being drawn.
Keywords
Cite
@article{arxiv.2508.01454,
title = {Error dependencies in the space-based CNEOS fireball database},
author = {Eloy Peña-Asensio and Hector Socas-Navarro and Darryl Z. Seligman},
journal= {arXiv preprint arXiv:2508.01454},
year = {2025}
}
Comments
Accepted in Astronomy & Astrophysics