Catastrophic disruption of asteroid 2023 CX1 and implications for planetary defense
arXiv:2509.12362 · doi:10.1038/s41550-025-02659-8
Abstract
Mitigation of the threat from airbursting asteroids requires an understanding of the potential risk they pose for the ground. How asteroids release their kinetic energy in the atmosphere is not well understood due to the rarity of significant impacts. Ordinary chondrites, in particular L chondrites, represent a frequent type of Earth-impacting asteroids. Here, we present the first comprehensive, space-to-lab characterization of an L chondrite impact. Small asteroid 2023 CX1 was detected in space and predicted to impact over Normandy, France, on 13 February 2023. Observations from multiple independent sensors and reduction techniques revealed an unusual but potentially high-risk fragmentation behavior. The nearly spherical 650 160 kg (72 6 cm diameter) asteroid catastrophically fragmented around 28 km altitude, releasing 98% of its total energy in a concentrated region of the atmosphere. The resulting shockwave was spherical, not cylindrical, and released more energy closer to the ground. This type of fragmentation increases the risk of significant damage at ground level. These results warrant consideration for a planetary defense strategy for cases where a >3-4 MPa dynamic pressure is expected, including planning for evacuation of areas beneath anticipated disruption locations.
This preprint has not undergone peer review (when applicable) or any post-submission improvements or corrections. The Version of Record of this article is published in \textit{Nature Astronomy}, and is available online at https://doi.org/10.1038/s41550-025-02659-8
References in corpus (8)
- PHOTOMETRYPIPELINE: An Automated Pipeline for Calibrated Photometry
- NEOMOD: A New Orbital Distribution Model for Near Earth Objects
- Two Strengths of Ordinary Chondritic Meteoroids as Derived from their Atmospheric Fragmentation Modeling
- SsODNet: The Solar system Open Database Network
- The January 7, 2015, superbolide over Romania and structural diversity of meter-sized asteroids
- A common origin for dynamically associated near-Earth asteroid pairs
- Stellar evolution models with overshooting based on 3-equation non-local theories, II. Main-sequence models of A- and B-type stars
- Aperture photometry on asteroid trails: detection of the fastest rotating near-Earth object
Cited by in corpus (6)
- Statistical significance of meteorite-asteroid pairs using geocentric parameters
- NEO and imminent impactor discoveries from Hungary: recent results and lessons learnt
- Predictions of Imminent Earth Impactors Discovered by LSST
- Consistency between dynamical modeling and photometrically derived masses of fireballs
- From orbit to ground: pre-impact meteorite strewn field predictions for imminent impactors and meteorite recovery
- A Near-Earth Object Model Calibrated to Earth Impactors