Abstract:
Knowing the likelihood of collision for satellites operating in Geosynchronous Earth Orbit (GEO) is of extreme
importance and interest to the global community and the operators of GEO spacecraft. Yet for all of its importance,
a comprehensive assessment of GEO collision likelihood is difficult to do and has never been done. In
this paper, we employ six independent and diverse assessment methods to estimate GEO collision likelihood.
Taken in aggregate, this comprehensive assessment offer new insights into GEO collision likelihood that are
within a factor of 3.5 of each other. These results are then compared to four collision and seven encounter rate
estimates previously published. Collectively, these new findings indicate that collision likelihood in GEO is as
much as four orders of magnitude higher than previously published by other researchers. Results indicate that a
collision is likely to occur every 4 years for one satellite out of the entire GEO active satellite population against a
1 cm RSO catalogue, and every 50 years against a 20 cm RSO catalogue. Further, previous assertions that collision
relative velocities are low (i.e.,<1 km/s) in GEO are disproven, with some GEO relative velocities as high
as 4 km/s identified. These new findings indicate that unless operators successfully mitigate this collision risk,
the GEO orbital arc is and will remain at high risk of collision, with the potential for serious follow-on collision
threats from post-collision debris when a substantial GEO collision occurs.
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D.L. Oltrogge, S. Alfano, C. Law, A. Cacioni, and T.S. Kelso, “A comprehensive assessment of collision likelihood in Geosynchronous Earth Orbit," Acta Astronautica (2018), doi:10.1016/j.actaastro.2018.03.017, also accessible at https://comspoc.com/Resources/Content/Private/C-20220422T165416/Paper/20180424_GEO_Collision_Risk_Paper_FINAL_Gold_Open_Access.pdf
