Using NSF’s Very Large Array (VLA), astronomers made the first radio detection of polarized light and Faraday rotation from a gamma-ray burst afterglow, offering an unprecedented glimpse of the magnetic fields surrounding one of the Universe’s most powerful explosions.
The post Astronomers Detect Gamma-Ray Burst’s Magnetic Fingerprint appeared first on Sci.News: Breaking Science News.
The molten iron core deep within our planet could be much more dynamic and complicated than previously known, as revealed in new studies that point to a current of liquid metal under the Pacific Ocean that reversed directions unexpectedly more than a decade ago.
The new findings provide additional insights into a sort of hidden “engine” driving the planet’s protective magnetic field, as detailed in new reporting featured in the Journal of Studies of Earth’s Deep Interior.
According to the research, long-held assumptions about large-scale flows occurring in Earth’s outer core are now being challenged, pushing back on previous notions that they evolve only gradually over time. Now, researchers say a broad region of molten iron beneath the equatorial Pacific abruptly shifted from a weak westward flow to a strong eastward current sometime around 2010.
Since our planet’s magnetic field is produced by the movement of superheated, electrically conductive liquid iron that is close to 2,200 kilometers (1,370 miles) below the surface, sometimes even the most nuanced changes within these deep currents can fundamentally alter the magnetic field that shields the planet from harmful charged particles emitted by the Sun.
Discovering this unexpected reversal required scientists to combine close to three decades of ground-based magnetic observations with satellite data collected from 1997 until 2025. The European Space Agency’s (ESA) Swarm Mission provided measurements, which, combined with previous observations made possible through German CHAMP and Danish Ørsted satellites, helped researchers behind the new work to construct a precise model of the changing flow patterns occurring at the boundary between Earth’s core and mantle.
“The large-scale flow reversal beneath the Pacific raises new questions about the behavior of Earth’s deep interior,” said lead author Frederik Dahl Madsen of the University of Edinburgh’s School of Geosciences.
“Scientists now want to understand whether the reversal represents a short-lived fluctuation, part of a repeating oscillation, or a new stable equilibrium for core circulation,” Madsen said.
Among their findings, the team also said they uncovered evidence that the strong eastward current appears to have weakened since 2020, raising the possibility that the reversal could represent part of a longer natural cycle.
According to Madsen, the shift coincided with changes inferred within Earth’s solid inner core, which suggests previously unrecognized links between the planet’s deepest layers.
“The rise of the strong eastward flow in the Pacific is contemporary with a change in behaviour in the inner core, as inferred from geodesy and seismology, and we hypothesize that these changes in the deep interior are associated with the changes in flow beneath the Pacific,” Madsen said.
While such processes occur thousands of kilometers beneath our planet’s surface and pose no direct dangers, they nonetheless have a vital part in sustaining Earth’s magnetic field.
Although invisible, the magnetic shielding capability it provides protects our atmosphere from solar radiation, while supporting the technologies many of us rely on daily for navigation, space weather monitoring and forecasting, and a range of other things.
ESA scientists say that in the long term, satellite missions like its Swarm mission provide a detailed picture of what’s happening in Earth’s hidden interior. That data is also revealing how the planet’s molten core may be considerably more variable and complex than once thought.
Going forward, Madsen says he and his colleagues will continue to look at how the molten flow deep within the earth is changing over time.
“Continued monitoring will be essential to determine how the flow evolves over the coming years,” Madsen said of the team’s ongoing work.
The team’s recent study, “Principal component analysis of the 2010 reversal of core-surface flow beneath the Pacific Ocean,” was published in the Journal of Studies of Earth’s Deep Interior.
Micah Hanks is the Editor-in-Chief and Co-Founder of The Debrief. A longtime reporter on science, defense, and technology with a focus on space and astronomy, he can be reached at micah@thedebrief.org. Follow him on X @MicahHanks, and at micahhanks.com.
An exoplanet is exerting a magnetic influence on its host star in a manner opposite to what astronomers normally observe, according to researchers at the Institute of Astrophysics of Andalusia (IAA-CSIC).
In a recent paper published in Science, IAA-CSIC researchers revealed how the exoplanet GJ 436 b is affecting its host star’s behavior in a never-before-seen way. In their work, the team developed a novel method to estimate an exoplanet‘s magnetic field strength, an important factor in determining habitability.
“Until recently it was thought that it was mainly the star that influenced the planet,” said Rafael Luque, an IAA-CSIC researcher and one of the new study’s co-authors.
Luque adds that his team’s results now offer “the clearest evidence to date of something that had already been suspected: that the opposite can also happen and that a nearby planet can alter the environment of its star.”
While the most obvious ingredients for a habitable planet are water and a breathable atmosphere, other elements are less apparent to us based on our human experience. Our planet’s invisible magnetic field protects us from the solar wind and holds the atmosphere together.
While Earth’s magnetic field guided the evolution of its atmosphere, Mars provides an example of what the loss of a magnetic field can do to an otherwise potentially habitable planet. When the Martian magnetic field disappeared four billion years ago as the planet’s core rapidly cooled, the atmosphere dissipated, followed by the loss of surface water.
As shown by the fates of two cosmic neighbors like Earth and Mars, a stable magnetic field is a key element of habitability.
Detecting magnetic fields on distant exoplanets has proven more challenging for astronomers than other observations, such as atmospheric composition. In their new paper, the IAA-CSIC team provides the first conclusive evidence of an exoplanet’s magnetic field, observed through its impact on the host star.
“In particular, we have observed that GJ 436 b, an exoplanet similar to Neptune that orbits very close to its star, causes regular changes in the brightness and energy emitted by the star at certain wavelengths,” explained lead author Daniel Revilla, an IAA-CSIC researcher who led the study as part of his doctoral thesis.
GJ 436 b provided the team with measurable signals that allowed them to infer that the exoplanet had a magnetic field and estimate its strength. The IAA-CSIC team analyzed sixteen years of spectroscopic observations of the GJ-436 system for their research, collected by the CARMENES instrument at the Calar Alto Observatory.
“Despite its smaller size, GJ 436 b would have a magnetic field between 2.33 and 27 times more intense than that of Jupiter,” said co-author Pedro J. Beloved, a researcher at the IAA-CSIC.
In the paper, the researchers demonstrate how, in a very close orbit, a planet can flip the normal planet-star relationship, with the planet controlling the influence of gravity, radiation, and magnetic fields between the two. As the exoplanet interacts with its host star, it injects energy into the star’s chromosphere to produce a phenomenon like a stellar aurora.
This strange interaction has only been measured periodically, occurring in eight-year cycles, with observations in 2008, 2016, and 2024. Intriguingly, these years correlate to phases of the host star’s magnetic cycle, which the researchers believe affects the intensity.
“Until now, measuring the magnetic field of an exoplanet was extremely difficult,” Devilla concluded. “This property is key to knowing if a planet can protect its atmosphere and, ultimately, if it could harbor life.”
The paper, “Constraining an Exoplanet’s Magnetic Field Using Star-Planet Interactions,” appeared in Science on June 25, 2026.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
A team of physicists set out to recreate a 60-year-old quantum mystery using a large water tank. While their experiment produced the expected results, it also revealed an unexpected behavior in the water.
The experiment centered on the Aharonov–Bohm effect, a strange quantum phenomenon where electrons respond to a magnetic field even when they never actually pass through it. First predicted back in 1959, this effect has been notoriously difficult to confirm because the changes it causes in electron waves are incredibly subtle.
Instead of using electrons and a particle accelerator, researchers from the Okinawa Institute of Science and Technology (OIST), along with collaborators in Oslo and Chile, recreated the effect using water waves, making an otherwise invisible quantum effect visible in a tabletop experiment. The team reported their findings in Communications Physics.
“With waves traveling the opposite direction, you see a mirror image pattern,” says Jonas Rønning, co- author and former postdoc in the OIST unit. “The question for us was, what happens if you send waves from both directions at the same time? We thought that the patterns might cancel each other out, or both pitchfork-like patterns would be visible, but our intuition was completely wrong.”
The researchers constructed a custom tank, created a vortex at its center, and sent waves from opposite sides to meet in the middle. They used a high-speed camera to observe how the waves interacted on the water’s surface.
Without a vortex, the peaks and troughs remain in place. When the vortex is there, the standing wave breaks down. The vortex shifts the phase of the waves as they travel around it, altering the standing-wave interference pattern and creating rotating nodal lines. These are lines of momentarily flat water that spiral outward and turn in the opposite direction of the vortex.
“This was something new and unexpected,” says Aditya Singh, a PhD student in the Nonlinear and Non-equilibrium Physics Unit and co-first author of the study. “That’s what makes this fluid analogue system so valuable. It reveals topological effects — wave behaviors that occur across the whole system — that can’t be seen in quantum experiments.”
At first, the team suspected their equipment was causing the rotating lines. However, the same pattern also appeared in their computer simulations.
“When we first saw these lines, we thought they were an experimental artifact,” Singh says. “But when we also saw them in our simulations, we dropped everything and quickly worked out the mathematics underlying how they arise.”
As the strength of the vortex increased, more rotating nodal lines appeared, always moving in the direction opposite to the vortex. The study showed that the number of lines is quantized, meaning it is fixed to whole-number values determined by the vortex’s circulation. In other words, the topology of the vortex determines how many rotating nodal lines appear. This effect was observed across the entire wave field, not just near the vortex core as earlier models suggested.
This finding differs from Berry’s original experiment, which observed changes only near the vortex. In this case, the researchers discovered a non-local effect, a pattern that covers the entire system and depends on the overall setup. Instead of being limited to the area near the vortex, the rotating nodal lines appeared throughout the whole standing-wave pattern.
Although the practical uses of these newly discovered nodal patterns are not yet clear, the study shows that simple classical systems can reveal behaviors that are challenging to observe in quantum experiments. By making these effects visible, the researchers plan to explore more complex wave systems that could offer new insights into superconductivity and other quantum phenomena.
“One direction is to make the system more complex by introducing multiple vortices and arranging them into a lattice,” senior author Mahesh Bandi says. “That setup would mirror conditions in some superconducting materials, with the water waves behaving like a supercurrent. We don’t yet know what we’ll see — and that’s exactly what makes it worth doing.”
Austin Burgess is a writer and researcher with a background in sales, marketing, and data analytics. He holds an MBA, a Bachelor of Science in Business Administration, and a data analytics certification. His work focuses on breaking scientific developments, with an emphasis on emerging biology, cognitive neuroscience, and archaeological discoveries.
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