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The Potential Danger to Satellites due to Ejecta from a 2032 Lunar Impact by Asteroid 2024 YR4 (2506.11217v1)

Published 12 Jun 2025 in astro-ph.EP, astro-ph.IM, and physics.pop-ph

Abstract: On 2032 December 22 the 60 m diameter asteroid 2024 YR4 has a 4% chance of impacting the Moon. Such an impact would release 6.5 MT TNT equivalent energy and produce a ~1 km diameter crater. We estimate that up to 108 kg of lunar material could be liberated in such an impact by exceeding lunar escape speed. Depending on the actual impact location on the Moon as much as 10% of this material may accrete to the Earth on timescales of a few days. The lunar ejecta-associated particle fluence at 0.1 - 10 mm sizes could produce upwards of years to of order a decade of equivalent background meteoroid impact exposure to satellites in near-Earth space late in 2032. Our results demonstrate that planetary defense considerations should be more broadly extended to cis-lunar space and not confined solely to near-Earth space.

Summary

  • The paper quantifies that a 2032 lunar impact could eject up to 10^8 kg of material, significantly increasing the risk to Earth-orbiting satellites.
  • It employs advanced numerical simulations to analyze crater formation, ejecta size distribution, and orbital dynamics with an estimated 10% delivery efficiency to Earth.
  • The study highlights the need for enhanced satellite protection and monitoring strategies to mitigate damage from concentrated meteoroid exposure.

The Potential Satellite Risks from Lunar Ejecta Following an Asteroid Impact in 2032

This paper investigates the potential ramifications for Earth-orbiting satellites if the asteroid 2024 YR4_4 impacts the Moon, an eventuality calculated to have a 4% probability of occurring on 22 December 2032. The authors explore the implications, with particular focus on the ejection of lunar material into cislunar space and the risks posed by this material to satellite constellations near Earth.

The anticipated impact would generate significant kinetic energy, equivalent to 6.5 megatons of TNT, resulting in a crater approximately one kilometer in diameter. Such impacts on the Moon are rare, estimated to occur every 5,000 years, emphasizing the significance of this potential event. The primary concern investigated is the possibility that a substantial mass of lunar ejecta, estimated at up to 10810^8 kg for particles above lunar escape velocity, could pose a danger to Earth’s near-orbit space environment.

Utilizing numerical simulations, the authors assess the potential effects of lunar ejecta of varying sizes, particularly the fluence of particles ranging from 0.1 to 10 mm. They postulate that, depending on the asteroid’s specific impact location, particularly if it strikes the trailing side of the Moon, the delivery efficiency of ejecta to Earth could be as high as 10%. This would result in meteoroid exposure for satellites that is equivalent to several years to potentially a decade of standard background impact exposure condensed into a short period in late 2032.

The paper identifies several key factors and methods for estimating the impact effects, including crater size estimation, the mass and speed of ejected material, the size frequency distribution of the ejecta, and the efficiency with which these particles might be delivered to Earth. Moreover, the authors simulate the ejected material's orbital dynamics using advanced numerical techniques to draw conclusions about the probable outcomes and threats posed to satellites.

The theoretical satellite risk assessments consider existing data on meteoroid impacts and determine that increased exposure from lunar ejecta could lead to accelerated degradation of satellite structures. The scale of the potential impact is significant, with predictions for impacts and consequent damage far exceeding typical annual exposure levels.

In anticipation of potential future developments, the paper suggests broadening planetary defense considerations beyond Earth to encompass cislunar space, given the demonstrated risks from impacts originating on celestial bodies such as the Moon. The paper also briefly touches on the implications for lunar surface operations and orbiting missions, emphasizing the potential danger of lunar ejecta even beyond direct impacts on the Earth.

Given the predicted increases in active satellite populations by 2032, the conclusions drawn necessitate careful consideration and enhanced modeling of satellite protectiveness against meteoroid impacts. This atmospheric and orbital risk factor could also serve as a stimulus for further studies into atmospheric sampling of potential debris originating from a lunar impact.

This comprehensive analysis of potential lunar impact consequences enhances understanding of the broader implications of celestial events not directly impacting Earth but significantly affecting its space environment. It underscores the need for comprehensive and anticipatory strategies in satellite fleet protection, as well as ongoing monitoring and possible observations from astronomical facilities to refine predictions and enhance preparedness for such eventualities.

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