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Reconnaissance and Mitigation Mission Options for Asteroid 2024 YR4Near-Earth asteroid 2024 YR4 was discovered by the Asteroid Terrestrial-impact Last Alert System (ATLAS) on 2024-12-27. Tracking showed a probability of Earth impact on 2032-12-22, peaking at 3.1% on 2025-02-18. By 2025-02-23, observations ruled out Earth impact, but the probability of lunar impact rose. Final observations during the discovery apparition were made by JWST on 202505-11. The probability of lunar impact is currently \~4.3%. The asteroid won't be visible from the ground again until June 2028 but may be detected by JWST again in early 2026. Wiegert et al (arXiv:2506.11217 [astro-ph.EP] 2025) estimate lunar impact debris could cause meteoroid flux in low Earth orbit reaching up to 1000 times background meteoroid flux (\~10 years of exposure) over just a few days, at sizes potentially hazardous to astronauts and spacecraft (> 0.1mm). Particles > 1 cm could lead to spacecraft disruption, creating more orbital debris.

In this work, we present options for space missions to 2024 YR4 that could be utilized to prevent a lunar impact, covering flyby & rendezvous reconnaissance, deflection, and robust disruption of the asteroid. We assess deflection requirements and compare them to current heuristics for onset of asteroid fragmentation. For robust disruption, we assess launch options for nuclear detonations and kinetic impactors, considering multiple heuristics for sizing missions to provide confidence of robust disruption. We evaluate chemical and solar electric propulsion (SEP) options, various launch vehicles, and optimized deep space maneuvers and gravity assists. Re-tasking of extant spacecraft and usage of built spacecraft not yet launched are also considered.

Though we find viable reconnaissance and mitigation trajectory options via our exhaustive search, the ~7 yr timeline is stressing. Viable responses either require reconnaissance mission development start prior to lunar impact probability reaching 100%, or require mitigation development start without the benefit of reconnaissance data. This is driven by 2024 YR4’s ~4 yr orbit period, which constrains spacecraft encounters to roughly 2028 and 2032. The use of large maneuvers or SEP can expand these windows at the expense of spacecraft complexity. We describe this trade space and present candidate responses that address constraints.
Document ID
20250008366
Acquisition Source
Goddard Space Flight Center
Document Type
Abstract
Authors
Brent W Barbee
(Goddard Space Flight Center Greenbelt, United States)
Justin Atchison
(Johns Hopkins University Applied Physics Laboratory North Laurel, United States)
Rylie Bull
(Johns Hopkins University Applied Physics Laboratory North Laurel, United States)
Wendy K Caldwell
(Los Alamos National Laboratory Los Alamos, United States)
Paul W Chodas
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Davide Farnocchia
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Dawn Graninger
(Johns Hopkins University Applied Physics Laboratory North Laurel, United States)
Megan Harwell
(Los Alamos National Laboratory Los Alamos, United States)
Patrick King
(Johns Hopkins University Applied Physics Lab)
Joshua Lyzhoft
(Goddard Space Flight Center Greenbelt, United States)
Ron Mink
(Goddard Space Flight Center Greenbelt, United States)
Catherine S Plesko
(Los Alamos National Laboratory Los Alamos, United States)
Adrienne Rudolph
(Goddard Space Flight Center Greenbelt, United States)
Matthew A Vavrina
(Goddard Space Flight Center Greenbelt, United States)
Date Acquired
August 13, 2025
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: American Geophysical Union (AGU) Annual Meeting
Location: New Orleans, LA
Country: US
Start Date: December 15, 2025
End Date: December 19, 2025
Sponsors: American Geophysical Union
Funding Number(s)
WBS: 582622.02.01.04.66
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
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