Voyager hits a 'Wall of Fire': NASA probe finds a furnace at the edge of the solar system

Time of India

18-06-2025

Voyager 1
has detected a shell of
superheated plasma
far beyond Pluto—offering a direct look at where the Sun's influence ends and
interstellar space
begins.
From nearly 24 billion kilometres away,
NASA
's ageing Voyager 1 has sent back a signal confirming one of the most extreme discoveries yet: a narrow region near the
heliopause
where plasma has been heated to an astonishing 30,000 to 50,000 Kelvin. This marks the latest in a string of insights from the 48-year-old spacecraft.
The heliopause, which defines the outer edge of the Sun's protective bubble known as the heliosphere, is where
solar wind
slams into material from interstellar space. It's not a wall in the traditional sense—but data show a sharp, localised zone of extreme temperatures.
by Taboola
by Taboola
Sponsored Links
Sponsored Links
Promoted Links
Promoted Links
You May Like
How Much Does It Cost to Rent a Private Jet - The Prices May Surprise You!
Private Jet I Search Ads
Learn More
Undo
An unexpected blaze in the cosmic borderlands
The discovery began with a spike in temperature data—despite the fact that Voyager 1's original plasma detector had failed years ago.
Instead, two other instruments still running—one monitoring cosmic ray hits, the other measuring the local magnetic field—spotted the clues. Solar wind ions dropped sharply. Meanwhile, cosmic ray counts surged and the magnetic field began to bend. That's when scientists realised what they were seeing.
Live Events
Researchers processed the data and saw evidence of a hot plasma shell, possibly just 1 astronomical unit thick. Hours later, Voyager 2—following its own path—picked up the same pattern, confirming the phenomenon wasn't a fluke.
'It's a narrow, searing frontier,' said NASA Heliophysics scientists. And the spacecraft sailed right through it.
What fuels a fire where nothing burns?
There's no flame out there. No oxygen to feed one. But the searing temperature comes from the collision of forces.
As the supersonic solar wind crashes into the slower-moving interstellar medium, magnetic turbulence and compression force particles into a higher energy state. That's where the heat comes from—particles zipping around at extreme speeds in a vacuum barely dense enough to warm aluminium.
In short: it's a cosmic blast furnace, but with so little matter that Voyager's hull doesn't heat up.
'She's been driving for five decades and just found the hottest rest stop in the universe,' quipped Suzanne Dodd, Voyager's flight director, after the data appeared on her Pasadena monitor.
A magnetic surprise beyond the Sun's reach
One of the biggest surprises wasn't the heat—but the alignment of
magnetic fields
.
Scientists expected the magnetic field outside the heliopause to change direction entirely. But both Voyager probes have found that the magnetic field beyond the boundary runs almost parallel to the one within the heliosphere.
NASA explained: 'An observation by
Voyager 2
's magnetic field instrument confirms a surprising result from Voyager 1: The magnetic field in the region just beyond the heliopause is parallel to the magnetic field inside the heliosphere.'
That's upended existing models of the Sun's protective bubble. It suggests the heliosphere may be more closely connected to the galaxy's magnetic environment than previously assumed—and that our cosmic shielding from high-energy radiation might work in ways still not fully understood.
This has important implications for protecting Earth and for long-duration human spaceflight.
The hottest postcard in Space
NASA's engineers remain in awe that Voyager 1 still works.
The data trickles in at just 160 bits per second. It takes 22 hours for a single message to arrive back at Earth's Deep Space Network.
'That silence after you send a command is the longest coffee break imaginable,' said Todd Barber, Voyager systems engineer.
Voyager's ageing plutonium battery can now only support a few instruments. But NASA has juggled power usage carefully to keep the most valuable sensors running. Even at 48 years old, the probe continues to report back from the unknown.
Next up: Mapping the edge in high definition
NASA is already planning the next step. In 2026, the Interstellar Mapping and Acceleration Probe (IMAP) will launch to observe the heliopause from within. It aims to capture the same plasma flows that Voyager just measured, but with modern instruments and clearer resolution.
Even further ahead is a proposed Interstellar Probe mission, designed to reach 400 AU in 50 years. Its goal? Map this fiery region—this 'invisible wall of fire'—in unprecedented detail.
All of this future planning leans on Voyager's current discoveries.
Voyager 1 crossed into interstellar space on 25 August 2012. Its twin, Voyager 2, followed in 2018. But even now, these machines keep pushing the boundaries of what humanity knows about the edge of its own solar neighbourhood.
Their findings aren't just scientific curiosities. They help shape real-world plans to shield astronauts from cosmic radiation and inform how Earth's magnetic defences operate.
In another dozen years, the last of Voyager 1's instruments may fall silent. But its final contribution—a message from the solar system's burning edge—might be its most important.
For now, it's still out there. Floating. Listening. Sending home the secrets of the stars.