A. S. Rivkin, J. de Wit, M. Micheli, D. Farnocchia, A. Y. Burdanov, B. Holler, D. J. Tholen, M. Devogele, D. Graninger, H. B. Hammel, S. N. Milam, T. Mueller, I. S. Narrett, Petr Pravec, C. A. Thomas
Abstract Asteroid 2024 YR4 poses no impact risk to Earth during its 2032 December 22 close approach (D. Farnocchia et al. 2026; M. Micheli et al. 2026). However, its projected probability of a lunar impact in 2032 has been approximately 4% since its last observation in late spring 2025. JWST observations in 2025 March and May constrained the size of 2024 YR4 to 60 ± 7 m (A. S. Rivkin et al. 2025). While this 60 m object does not threaten Earth directly, a lunar impact of this scale could affect the reliability and resilience of Earth–Moon orbital infrastructure (P. Wiegert et al. 2025; Y. He et al. 2026), and is of additional interest due to the possibility of human exploration at that time. New astrometric measurements obtained with JWST/Near Infrared Camera on 2026 February 18 and 26 extend the observational arc by eight months and reduce the 2032 lunar B-plane uncertainty by more than an order of magnitude. These measurements demonstrate that 2024 YR4 will pass at 22,900 ± 800 (1 σ ) km from the center of the Moon, thus ruling out a lunar impact, in agreement with the official assessments by NASA ( https://science.nasa.gov/blogs/planetary-defense/2026/03/05/new-nasa-asteroid-observations-eliminate-chance-of-2032-lunar-impact/ ) and ESA ( https://www.esa.int/Space_Safety/Planetary_Defence/Asteroid_2024_YR4_will_not_impact_the_Moon ). The JWST team achieved this refinement approximately two years in advance of the next possible ground-based recovery of the asteroid, materially advancing the timeline for hazard assessment. The sequence of infrared size determination followed by deep-space astrometric orbit refinement illustrates the operational role JWST and future facilities like the Habitable Worlds Observatory (J. Dotson et al. 2025) can play in precision planetary-defense assessments for faint ( V mag < 31), decameter-scale near-Earth objects beyond the reach of ground-based facilities.