The longest solar burst ever detected lasted nearly three weeks, according to a new study published in The Astrophysical Journal Letters. The event, a type IV solar burst, persisted for 19 days—from August 21 to September 9, 2025—shattering the previous record of five days.
Four spacecraft had to combine their observations to confirm and study the phenomenon. The European Space Agency's Solar Orbiter first spotted the burst, and NASA's Wind and Parker Solar Probe later confirmed it, with STEREO-A adding further support.
What Is a Type IV Solar Burst?
A solar burst occurs when electrons become trapped in the Sun's magnetic field and spiral around its field lines, emitting intense electromagnetic radiation. There are five known types of solar bursts, each with distinct characteristics.
Type IV bursts are particularly notable for their broad bandwidths and long durations. They often signal the presence of large-scale magnetic structures in the solar corona, which can be important for understanding space weather.
How the Record-Breaking Burst Was Detected
The Solar Orbiter, designed to study the Sun's poles, solar wind, and magnetic field from close range, made the initial detection. It had observed many solar bursts before, but never one with these characteristics.
Twelve days later, NASA's Wind and Parker Solar Probe confirmed the finding. A few days after that, STEREO-A provided additional confirmation. The multi-spacecraft approach was crucial for validating such an extraordinary event.
Why This Solar Burst Matters
This record-breaking burst provides new insights into the Sun's magnetic behavior and the processes that drive long-lasting solar emissions. Understanding these events is key to predicting space weather, which can affect satellites, power grids, and astronaut safety.
The 19-day duration suggests that the underlying magnetic structures remained stable for an unusually long time, offering a rare opportunity to study how energy is released and sustained in the solar corona.
- The burst lasted 19 days, far exceeding the previous 5-day record.
- Four spacecraft—Solar Orbiter, Wind, Parker Solar Probe, and STEREO-A—confirmed the event.
- Type IV bursts are characterized by broad bandwidths and long durations.
- Studying such events helps improve space weather forecasting.
- The finding was published in The Astrophysical Journal Letters.
Comparing Solar Burst Types
Solar bursts are classified into five types based on their radio signatures. The table below summarizes the key features of each type, with type IV being the focus of this record-breaking event. The background to this story is set out in Farthest Fast Radio Burst Ever Detected Reveals Early Universe Secrets. A related thread runs through First Radio Waves Detected from an Exoplanet: What It Means. Earlier coverage in What Is a Thermal Burst and Why It Threatens the Mediterranean shows how the argument developed.
| Type | Duration | Key Characteristics |
|---|---|---|
| Type I | Seconds to minutes | Narrowband, often associated with active regions |
| Type II | Minutes to hours | Slow drift, linked to shock waves |
| Type III | Seconds to minutes | Fast drift, electron beams |
| Type IV | Hours to days | Broadband, long-lasting, trapped electrons |
| Type V | Minutes | Short-lived, associated with type III |
What to Watch Next
Researchers will continue to analyze data from this event to better understand the mechanisms behind such long-duration bursts. Future missions, including the recently launched Aditya-L1 and the upcoming PUNCH mission, will provide additional viewpoints. A closer look at the same subject appears in SpaceX Starship Reaches Orbit for the First Time Ever. Anyone following the wider picture can start with NASA's Fire-Detecting Satellite Plagued by Space Junk. The same theme surfaces in Science: latest articles, which takes a different angle.
As the Sun approaches the peak of its current activity cycle, more extreme events are likely. Keeping an eye on space weather forecasts will be important for anyone reliant on satellite technology. Context on how this played out before sits in SMILE Mission Launch: When We'll See Its First Data.
FAQ
What is a solar burst?
A solar burst is a sudden release of electromagnetic radiation from the Sun, often caused by electrons spiraling in the solar magnetic field. These bursts are observed at radio wavelengths and can last from seconds to days.
How long did the longest solar burst last?
The longest solar burst ever recorded lasted 19 days, from August 21 to September 9, 2025. It was a type IV burst, which are known for their long durations.
Which spacecraft detected the record-breaking burst?
The burst was first detected by the European Space Agency's Solar Orbiter. NASA's Wind and Parker Solar Probe confirmed it, and STEREO-A provided additional support.
Why is this discovery important?
Understanding long-duration solar bursts helps scientists learn more about the Sun's magnetic field and improve space weather predictions, which can protect satellites and power grids.