Researchers have simulated using a 1-megaton nuclear warhead against a 160-metre-wide asteroid to test Earth-defense options against late-discovered threats. Led by astrophysicist Isaiah Santistevan, the computer models explored how X-ray energy and shock waves could break apart an impactor too close for conventional deflection.
The concept of deploying atomic weapons against hazardous space rocks is decades old, but modern computing has allowed teams to test the physics in high detail. Researchers from Lawrence Livermore National Laboratory turned to powerful computer simulations to examine what happens when a 1-megaton nuclear device is detonated near a threatening object using 3D modeling based on real-world meteorite data and structural profiles.
Simulating a Nuclear Strike on a 160-Metre Asteroid
The study, published in The Planetary Science Journal under the title ‘Nuclear Mitigation of Hypothetical Asteroid Threats in Smoothed Particle Hydrodynamics’, focused on an object roughly 160 metres wide, or about 525 feet across according to the research details. An asteroid of this scale is comparable in size to a football field and possesses enough kinetic energy to cause devastating urban or regional destruction if it hits populated ground. The ideal planetary-defence scenario would be to detect a dangerous object far enough in advance to change its trajectory by a tiny amount, allowing an asteroid to pass harmlessly past Earth rather than striking it. Some objects can be difficult to detect, particularly dark asteroids that reflect little sunlight, while a relatively short warning time could leave scientists with far fewer options. The researchers’ simulations were designed to explore precisely that last-resort possibility rather than suggest that nuclear weapons should be the first choice for planetary defence.

Led by astrophysicist Isaiah Santistevan of Lawrence Livermore National Laboratory, the team modeled three distinct scenarios to see whether the blast could break the body apart and how the resulting fragments would travel. The simulations established that nuclear disruption could be highly effective in two of the three tested scenarios, giving scientists a potential last-line defense when gentler deflection methods fail. The findings also highlight how the effectiveness of a nuclear response would depend heavily on the asteroid’s structure, composition and the timing of the intervention.
How X-Ray Energy and Shock Waves Break Space Rocks
The mechanics of a nuclear defense option differ fundamentally from Hollywood depictions. The weapon does not need to collide directly with the asteroid. Instead, the models showed that detonating the device several metres away from the surface unleashes a massive wave of X-ray energy.
Around 70 to 80 per cent of the energy from a nuclear explosion emerges as X-rays in these physical models. That intense radiation heats the asteroid’s outer layer so violently that surface material vaporizes and blasts outward, creating a jetting effect that alters the body’s speed and trajectory.
Simultaneously, the blast drives powerful shock waves deep into the interior, cracking the structure apart. To ensure realism, the team based their simulated asteroid’s porous structure on Bennu—the target of NASA’s OSIRIS-REx mission—while integrating compositional data from the Chelyabinsk meteorite that exploded over Russia in 2013 and the Aba Panu meteorite that fell in Nigeria in 2018.
Computational Demands and Remaining Uncertainties
In one simulation where the detonation occurred 10 metres above the surface, roughly 98.2 per cent of the material sustained heavy damage, while around 97 per cent moved faster than the asteroid’s escape velocity as detailed in the test results. Moving the detonation point out to 25 metres unexpectedly produced even more widespread damage at specific points during the model run.
Yet simply breaking an asteroid apart introduces its own hazards, as a botched fragmentation can scatter numerous dangerous chunks toward Earth instead of one massive body. Tracking every fragment long-term remains an immense computational hurdle. One of the longest simulation runs covered a physical span of just 145 milliseconds yet required 59 days to compute across 1,680 processors, leaving the ultimate fate of individual fragments unmapped past the initial blast.
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