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Predicting Space Weather Is Possible—Could We Also Stop It?

3 June 2026 at 19:53

The weather on Earth can get pretty messy sometimes. But in space, it can be wild—and the effects can be far-reaching.

Solar flares, giant explosions on the sun, can send out streams of energy that block radio communications and fry satellite electronics. Geomagnetic storms, caused by variations in solar wind, can mess with GPS signals and spark current surges on Earth that overload power grids.

The impact of space weather isn’t limited to temporarily losing electricity or digging out dusty paper maps for directions when satellite navigation systems fail. Every electronic financial transaction in the world, for instance, relies on time stamps sent by satellite systems. And, in May 2024, a solar storm threw out GPS systems used to accurately guide tractors in planting and harvesting crops, hobbling food production for days and costing US farmers $500 million.

Although satellites can be built with tougher shields or have their orbits adjusted, those are just Band-Aids; there’s currently little we can do to protect ourselves from space storms.

Boston University researcher Brian Walsh has an idea for how to change that. He’s been testing the theoretical feasibility of a system of spacecraft that could fire chemical elements to the edge of Earth’s magnetic field, temporarily fortifying our defenses and deflecting potentially damaging space weather. In simulations, Walsh and researchers from the University of Michigan found the system could cut the intensity of a major geomagnetic storm in half. The findings were published in the journal Space Weather.

“Since humans have been in space, we’ve been trying to predict what’s going to happen in the space environment,” says Walsh, a BU College of Engineering associate professor of mechanical engineering. “But we came up with a model that could flip the paradigm. It’s like people in a village who see a river flooding—maybe they can predict when that will happen, but probably what’s even better is if they could build a storm wall. That’s what we’re proposing here.”

Bouncing Storms Past the Earth

Walsh says his idea for a weather wall in space was inspired by a natural phenomenon: material peeling off the Earth’s atmosphere and floating to the edge of our planet’s protective bubble, the magnetosphere, to bolster it. “I thought, maybe you could turn [that process] up, increase the intensity of it,” he says.

His proposed system, named StormWall, would start with the launch of six spacecraft into a geosynchronous orbit matching the Earth’s own rotation. Each craft would be fitted with a canister loaded with what the researchers call a mass-loading material. When released, the material—an alkaline chemical element like barium or lithium—would photoionize, a process that induces an electrical charge, seeding the atmosphere with plasma.

In their simulations, Walsh and his colleagues found that this plasma would disrupt the flow of energy between any solar storm and the magnetosphere—and that would be enough to bounce the space weather around and past our planet.

Not Science Fiction

Walsh admits a weather wall in space sounds a little like science fiction, but says it’s within our reach.

“When you apply some really serious physics to it, it does work. And the amount of mass we need, the launch capacities—it’s all within our capabilities,” he says. “People have always thought, ‘space is huge, the sun is massive, we just have to sit here and take whatever it gives us.’ But what we found is that we can impact it.”

One of the biggest barriers to implementation is cost. Launching six spacecraft, together carrying the equivalent of about a dozen oil trucks–worth of material, wouldn’t be cheap. And once the payload is fired out and photoionizes, the system would be dead and couldn’t be replenished—it’s one and done. But with private companies investing billions in space infrastructure—and even contemplating data centers in orbit—Walsh says the math on cost-benefit ratios could soon favor his proposed approach. In their paper, Walsh and his colleagues point out that a massive once-in-a-century geomagnetic storm—the last one was in 1859—would cause devastating damage in space and on Earth, with power grid costs alone topping $2.4 trillion.

He’s confident the team can bring down the StormWall costs too. Next on their agenda is studying ways to half the material used, simulating a pulsed release of materials to extend the system’s lifespan, and examining potentially more efficient orbits. They also want to dig deeper into the chemistry involved to nail down the best elements to use.

And although space junk is a major issue in Earth’s lower atmosphere, Walsh says any materials they pump into its higher reaches would quickly be carried out of the system after they’ve done their job. “The material drifts out on these natural highways, it leaves the system—the magnetosphere flushes the material out within six or so hours.”

Geoengineering Space

As the head of BU’s Space Physics & Technology Lab, much of Walsh’s broader research is focused on observing and better understanding the space environment around Earth; he and his team were recently part of a mission that sent a telescope to the moon to image our magnetic shield. Although the StormWall project is loosely connected to that wider work, Walsh says it’s a bit of an outlier. “This is quite different than what anyone is doing right now—I don’t know of anyone proposing to geoengineer space.”

Should the idea literally take off, he says that, unlike some space missions that might reap rewards for the few, this one would benefit us all.

“If you built it, if it was deployed, it would help all people on the planet,” says Walsh. “You couldn’t make it in a way that helped only one country, one group of satellites.”



Journal

Space Weather

Method of Research

Computational simulation/modeling

Subject of Research

Not applicable

Article Title

Terrestrial Space Weather Protection Through Human-Produced Mass-Loading

Article Publication Date

2-Jun-2026

COI Statement

The authors declare no conflicts of interest relevant to this study.

Media Contact

Jennifer Rosenberg

Boston University

jennr@bu.edu

Journal
Space Weather
Funder
U.S. National Science Foundation
DOI
10.1029/2025SW004846

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One of America’s Rarest Species Just Narrowly Survived a Historic Wildfire—NASA Satellite Images Reveal the Stunning Damage

3 June 2026 at 16:10

Newly released NASA satellite images reveal the extent of recent wildfire damage on Santa Rosa Island in vivid detail, showcasing the impact of the largest Channel Islands fire on record.

The images, obtained with NASA satellite observation platforms that include the Fire Information for Resource Management System (FIRMS) and the Fire Event Explorer, reveal fire damage to nearly half of the island’s southeastern side.

The fire was initially spotted on May 15, 2026, and containment efforts began as the blaze spread across the island over the following days.

Now, the new NASA imagery is revealing the extent of the damage caused by the historic fire, which officials say came close to endangering one of our nation’s rarest species.

Channel Islands
California’s Channel Islands, with Santa Rosa Island visible in the center. Fire damage is visible on the island’s southeastern portion (Image Credit: NASA Earth Observatory/Lauren Dauphin, using Landsat data from the U.S. Geological Survey).

18,000 Acres Scorched on Santa Rosa Island

Current damage estimates indicate that close to one-third of the island was impacted, constituting more than 18,300 acres on the island, which is part of California’s Channel Islands National Park.

Comparisons with past NASA imagery of Santa Rosa Island, made possible with Landsat satellite images, reveal a sharp contrast between once verdant regions of the island, which are now scorched by fire, shown in reddish brown in the more recent images (see below).

Santa Rosa Island fire
Santa Rosa Island is shown in a side-by-side comparison, featuring the wildfire near its outset on May 16, 2026, and subsequent imagery from May 24, 2026, as the fire spread across approximately 1/3 of the island (Image Credit: NASA Earth Observatory/Lauren Dauphin, using Landsat data from the U.S. Geological Survey).

Fortunately, Channel Islands National Park officials reported that the fire had been 97 percent contained by May 26, after burning its way through chaparral and grassland covering large portions of the island.

Endangering One of America’s Rarest Species

The Channel Islands serve as a unique and extremely diverse habitat for a range of species of both plants and animals. Among the species threatened during the recent fires were Torrey pines (Pinus torreyana), recognized as our nation’s rarest pine tree, which only grows on Santa Rosa Island and in a preserve in urban San Diego.

Torrey pines
A wild grove of Torrey pines on Santa Rosa Island (Image Credit: Wikimedia Commons/CC BY 2.5).

Fortunately, most of the island’s Torrey pine forest remains intact, although some damage was reportedly discernible in surveys by firefighters on the island and in drone imagery of the scorched areas.

According to island officials, the fire appears to have burned its way inland at lower intensity, making its way through pine areas that burned ground-dwelling vegetation while leaving the overlying canopy largely unaffected.

Damage from the Largest Channel Island Fire

Park officials say that some smaller areas of forest did sustain significant damage, as conditions in those pockets allowed a greater burn intensity.

Closer to the fire’s northern boundary, Santa Rosa’s cloud forests—the wooded areas comprised mostly of oak and pine growth surrounded by chaparral, whose name is derived from the island fog that sustains them—were successfully preserved by firefighting crews who worked ahead of the fire to cool areas where combustible vegetation grows.

Based on recent local reports, the fire that consumed large portions of Santa Rosa Island’s vegetation is the largest known to have impacted any of the Channel Islands. Fortunately, many of the island’s indigenous trees and other vegetation are resilient enough to withstand fire, since they do not rely on it as part of their growth cycles like many mainland plant species.

Additional information about the fires can be found here, and more imagery of the recent damage has been made available at NASA’s Earth Observatory page.

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.

Scientists Discover an Astronomical ‘Rosetta Stone’ for Decoding Mysterious Cosmic Signals

3 June 2026 at 12:59


An international team of astronomers has uncovered what they are calling the clearest evidence yet for dying white dwarf stars as the origin of a class of mysterious cosmic signals called long-period radio transients.

The research, led by University of Sydney PhD student Kovi Rose, potentially offers researchers a ‘Rosetta Stone’ capable of deciphering and categorizing other such signals.

“For the first time, we have pinpointed the origin of these signals, confirming the source to be a ‘cataclysmic variable’, or an accreting white dwarf star,” Rose explained in an email to The Debrief.

The team behind the discovery, including the astronomers at CSIRO’s ASKAP radio telescope, said that identifying the origin of these transient cosmic signals that come from a few remote regions of the Milky Way galaxy could also offer researchers a “natural laboratory” to study the extreme physics that occur in such environments.

Mysterious Cosmic Signals “Have Puzzled Astronomers for Years”

According to the same email, long-period radio transients were initially thought to be slow-spinning neutron stars, known as pulsars, emitting periodic energy bursts. However, the team notes that mathematical models suggest that slow-rotating neutron stars cannot generate enough energy to produce the mysterious cosmic signals.

“Long-period radio transients have puzzled astronomers for years,” Mr. Rose explained. “We’ve only found about a dozen, and their origins have been unclear.”

Hoping to solve the mystery, the University of Sydney-led team aimed their instruments at a region of space and discovered a small, dense star called a white dwarf. However, unlike our solitary Sun, this white dwarf is part of a binary star system, named ASKAP J1745−5051, with a much larger but less dense red dwarf as its companion.

mysterious cosmic signals
Artists’ impression of a white dwarf binary system, ASKAP J1745-5051, that could serve as a cosmic ‘Rosetta Stone’ for studying long-period radio transients. Image Credit: Carl Knox/OzGrav/Swinburne & Joshua Preston Pritchard (CSIRO).

After several scans with ASKAP, the team discovered that the smaller white dwarf, about the size of Earth but with a mass closer to the Sun’s, was shedding or accreting material onto the larger but less dense red dwarf star. As the material heats up, it releases X-rays.

The team also detected periodic bursts of radio signals from the binary system. Although these regular emissions are tied to the system’s orbital motion, the researchers found that the bursts of X-rays and radio signals didn’t peak at the same time. According to Mr. Rose, this lack of synchronicity “tells us they’re being produced in different regions of the system.”

Analysis Reveals Long-Period Radio Transient Match

A closer analysis suggested that, due to the proximity of the two stars, which orbit each other in just one hour, their interacting magnetic fields were producing regular radio-wave bursts, which the team clocked at 1.4-hour intervals.

Professor Murphy, Head of School at the University of Sydney School of Physics and Chief Investigator at the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), said that similar objects have previously been linked to binary star systems, “but this is the first one where we can clearly see both stars and the accretion process in action.”

When the team compared the emissions from the binary system with those of previously detected long-period radio transients, the data were a clear match. According to Rose, this comparison proved definitively that this elusive category of mysterious cosmic signals “comes from a white dwarf actively pulling material from a companion star.”

Natural Laboratories for Exploring Extreme Plasma Physics

Although the team’s findings do not rule out other causes of these mysterious cosmic signals, they said their discovery “strengthens an alternative explanation” that at least some are caused by binary star systems involving white dwarfs.

“The system is also only the second known long-period radio transient to emit regular X-rays – and the first where the cause of the regularity has been confirmed,” they explained.

When discussing the potential impact of their findings on future research, the team noted that ASKAP J1745-5051 could provide astronomers “a reference point” for understanding other long-period radio transients that have remained uncharacterized.

Mr. Rose said that the system could help researchers determine whether other long-period transients are more like pulsars or like white dwarf systems, “acting like a stellar Rosetta stone,” referencing the famous stone tablet that helped modern researchers decipher Egyptian hieroglyphs. He also noted that the system offers researchers a unique opportunity to study extreme plasma physics and magnetic-field interactions “under conditions that cannot be replicated on Earth.”

“These systems are natural laboratories,” Mr Rose said. “They allow us to test our understanding of how matter behaves in strong magnetic fields and under intense gravitational forces.”

In the future, the University of Sydney-led team said they are planning future observations of the system with a combination of optical, radio, and X-ray telescopes “to better understand how these emissions are generated” and to determine whether similar mechanisms found in this system can explain the full population of long-period radio transients spotted to date.

“Each new discovery is helping us piece together the bigger picture,” Mr Rose explained. “We’re only just beginning to understand this new class of cosmic events.”

The findings are published in the journal Nature Astronomy.

 Christopher Plain is a Science Fiction and Fantasy novelist and Head Science Writer at The Debrief. Follow and connect with him on X, learn about his books at plainfiction.com, or email him directly at christopher@thedebrief.org.

Muon Space unveils Starship-class satellite platform for orbital data centers

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New laser-treated metal could help keep satellites cool in space

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The post New laser-treated metal could help keep satellites cool in space appeared first on Knowridge Science Report.

Astronomers Detect a Close Pair of Supermassive Black Holes for the First Time

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How long will it take to rebuild Blue Origin's launch pad? We asked some SpaceX vets.

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Nearly a decade later, on May 28, Blue Origin conducted a static fire test of a new rocket, with its larger New Glenn vehicle a few miles down the Florida coast. The company had gotten further into its test, reaching engine ignition, before its rocket also exploded.

Read full article

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How long will it take to rebuild Blue Origin's launch pad? We asked some SpaceX vets.

3 June 2026 at 11:00

A former NASA engineer named John Muratore sat on console as launch director in early September 2016 as propellant flowed onto a Falcon 9 rocket in Florida. Ahead of a planned launch two days later, SpaceX was preparing for a static fire test of the vehicle.

Then, all of a sudden, the rocket exploded. "It came out of nowhere, and it was really violent," Muratore said. This fireball resulted in the destruction of the rocket, much of its launch site, and the AMOS-6 satellite already attached to the vehicle.

Nearly a decade later, on May 28, Blue Origin conducted a static fire test of a new rocket, with its larger New Glenn vehicle a few miles down the Florida coast. The company had gotten further into its test, reaching engine ignition, before its rocket also exploded.

Read full article

Comments

© USLaunchReport

How long will it take to rebuild Blue Origin's launch pad? We asked some SpaceX vets.

3 June 2026 at 11:00

A former NASA engineer named John Muratore sat on console as launch director in early September 2016 as propellant flowed onto a Falcon 9 rocket in Florida. Ahead of a planned launch two days later, SpaceX was preparing for a static fire test of the vehicle.

Then, all of a sudden, the rocket exploded. "It came out of nowhere, and it was really violent," Muratore said. This fireball resulted in the destruction of the rocket, much of its launch site, and the AMOS-6 satellite already attached to the vehicle.

Nearly a decade later, on May 28, Blue Origin conducted a static fire test of a new rocket, with its larger New Glenn vehicle a few miles down the Florida coast. The company had gotten further into its test, reaching engine ignition, before its rocket also exploded.

Read full article

Comments

© USLaunchReport

NASA’s Fermi Telescope Caught a Supernova Doing Something Never Seen Before

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