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BepiColombo Makes Up-Close Measurement of Mercury's Solar Bombardment
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BepiColombo Makes Up-Close Measurement of Mercury's Solar Bombardment

BepiColombo's measurements of particle bombardment at Mercury will help assess the impact of space storms on Mercury's surface and on Earth's atmosphere.

Original source cited and editorially framed by Cosmos Week. Universe Today
Editorial signatureCosmos Week Editorial Desk
Published19 Sep 2026 02: 19 UTC
Updated2026-09-19
Coverage typeScience journalism
Evidence levelJournalistic coverage
Read time4 min read

Key points

  • Focus: BepiColombo's measurements of particle bombardment at Mercury will help assess the impact of space storms on Mercury's surface and on Earth's
  • Detail: Science reporting: verify primary technical documentation
  • Editorial reading: science reporting; whenever possible, verify the cited primary source.
Full story

BepiColombo's measurements of particle bombardment at Mercury will help assess the impact of space storms on Mercury's surface and on Earth's atmosphere. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.

This matters because physics only takes a result seriously when the measurement chain remains robust under scrutiny. Experimental particle physics and precision metrology both operate in regimes where the signal sits far below the background noise, and where systematic uncertainties can mimic new physics if not controlled rigorously. The history of the field contains numerous anomalies that generated theoretical excitement before better data showed them to be artifacts, and it also contains genuine discoveries that were initially dismissed as noise. The difference is almost always resolved by independent replication with different instruments and different systematics. During the eight years since it was launched, the ESA/JAXA BepiColombo mission has made six close flybys of Mercury. During the mission's fourth flyby in September 2024, this instrument detected how particles from a solar eruption penetrated Mercury's magnetic field and impacted the surface.

In a new study published in Nature Astronomy, a team led by researchers from the University of Helsinki showed how these results could inform predictions of space weather. As she and her colleagues noted, BepiColombo 's fourth pass of the planet - on September 4th 2024 - brought the mission within just 165 km (102.5 mi) of the planet’s surface.

This coincided with elevated fluxes of high-energy charged solar particles, giving astronomers the opportunity to study how planets close to their stars shield themselves. The spacecraft came much closer to the surface than it will be on its final orbit, and we were lucky that a major particle eruption occurred on the Sun at exactly that moment.

The results could therefore help inform predictions of space weather and its potential impact on Earth. Said co-author Rami Vainio, the co-Principal Investigator of SIXS and a professor of space physics at the University of Turku: Mercury's magnetic field is weaker than Earth's, and.

The broader interest lies as much in the method as in the headline number, because a durable measurement procedure can travel farther than a single result. When experimental physicists develop a technique that achieves new sensitivity or controls a previously uncharacterized systematic, that methodological contribution persists even if the specific measurement is later revised. This is one reason why precision physics experiments often generate long-term value that is not immediately visible in the original publication.

SIXS's observations help us assess how destructive particle radiation would penetrate Earth's near-space environment and atmosphere during the most powerful space storms. The SIXS observations will also be used in the Center of Excellence in Space Resilience, a program dedicated to ensuring that commercial and scientific operations in Low Earth.

Because this item comes through Universe Today 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 more measurement, tighter systematic control and scrutiny from groups whose experimental setups are genuinely independent. In experimental particle physics and precision metrology, the threshold for a discovery claim is a five-sigma excess surviving multiple analyses; an intriguing signal at lower significance is a reason to run more experiments, not a reason to revise the textbooks. Next-generation experiments currently under construction or commissioning will revisit several of the open questions that give the current result its context.

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