Predicted Ejecta Dynamics and Observability of the 2026 Falcon 9 Upper Stage Lunar Impact
William Jo, David B. Goldstein, Philip L. Varghese, Laurence M. Trafton, Jordan K. Steckloff, Arnaud Mahieux
astro-ph.EP
Submitted: 2026-07-27
Comments: Submitted to Astronomy & Astrophysics. 10 pages (7 main text + 3 appendices) (August 4th, 2026). Previously submitted to Geophysical Research Letters (July 2026)
Project page: https://isale-code.github.io
License: http://creativecommons.org/licenses/by/4.0/
The gist: On Aug.
Terminology
Abstract
On Aug. 5 at 06:34 UTC, a Falcon 9 upper stage (3,900 kg) will strike the lunar surface at 2.43 km/s, yielding a potentially visible debris plume. We present a study of the expected impact dynamics and resulting possibly observable debris field. The debris plume should reach roughly 15 to 20 km in altitude for the ejecta curtain and 75 to 100 km for the central ejecta spike, extend 183 km laterally from the impact point near the sunlit limb, and yield a peak dust column density above 10 km altitude of 6.08*10 7 m-2. Simulated I/F exceeds dark-sky background brightness by several orders of magnitude for the first few minutes after impact, reaching I/F = 1.27*10-3 at the earliest resolved time (t = 5 s). Above 10 km, peak I/F reaches 1.33*10-5, still several orders of magnitude brighter than the dark sky.
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