Cosmos Week
An asteroid's shape influences where a nuclear blast must be aimed to deflect it
Earth scienceEnglish editionScience journalismJournalistic coverage

An asteroid's shape influences where a nuclear blast must be aimed to deflect it

If a dangerous asteroid were headed toward Earth, one defense could be a nuclear detonation to blast one side with X-rays and nudge it off course.

Original source cited and editorially framed by Cosmos Week. Phys. org Space
Editorial signatureCosmos Week Editorial Desk
Published03 Nov 2026 16: 20 UTC
Updated2026-11-03
Coverage typeScience journalism
Evidence levelJournalistic coverage
Read time4 min read

Key points

  • Focus: If a dangerous asteroid were headed toward Earth, one defense could be a nuclear detonation to blast one side with X-rays and nudge it off course
  • Detail: Science reporting: verify primary technical documentation
  • Editorial reading: science reporting; whenever possible, verify the cited primary source.
Full story

If a dangerous asteroid were headed toward Earth, one defense could be a nuclear detonation to blast one side with X-rays and nudge it off course. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.

The significance lies in Earth science becomes stronger when local observations can be placed inside a broader physical pattern that spans time and geography. The planet operates as a coupled system in which atmospheric, oceanic, cryospheric and solid-Earth processes interact across timescales from days to millions of years. A measurement that captures one variable at one location and one moment has limited interpretive value until it is embedded in the longer series and wider spatial coverage that allow natural variability to be separated from forced change. This article has been reviewed according to Science X's editorial process and policies. Craig Fritz If a dangerous asteroid were headed toward Earth, one defense could be a nuclear detonation to blast one side with X-rays and nudge it off course.

But new simulations suggest that for a lumpy, irregular asteroid, exactly where those X-rays hit could make a huge difference. In a study published in Icarus, researchers found that irradiating different sides of the same simulated asteroid changed how much momentum the blast imparted and how much spin it.

What surprised us was how much. " For a different asteroid, the change in its rotational speed after deflection, how fast it spun, varied by a factor of 17. The new simulations offer the most detailed look yet at the asteroid deflection problem.

Our new algorithm is over 1, 600 times faster, which was critical to this breakthrough," Moore said. With the old models, computers just couldn't handle it. " Moore has been studying the issue of accurate modeling since an experiment at Sandia's Z machine showed, for the first.

The broader interest lies in linking the observation to climatic, geophysical or environmental dynamics that extend well beyond the immediate event or location. Earth science is unusual in that its most important questions operate on timescales that no single research career can observe directly, making the archival record, whether in ice, sediment, rock or satellite data, as important as any new measurement. Results that can be embedded in that record, and that either confirm or challenge the patterns it reveals, carry disproportionate scientific weight.

The key innovation here was figuring out how to combine the two simulation approaches. " Discover the latest in science, tech, and space with over 100, 000 subscribers who rely on. The simulations let researchers model an asteroid based on high-resolution 3D imagery from spacecraft flybys, then simulate effects from an X-ray burst while tailoring the size.

Because this item comes through Phys. org Space as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.

The next step is to place the result inside longer time series and to compare it with independent instruments and independent sites. Earth system observations gain most of their interpretive power from network density and temporal depth, not from any single measurement however precise. Model simulations that assimilate the new data will help clarify whether the observation fits comfortably within known natural variability or represents a shift that existing models do not reproduce.

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