Space · Article
Record-breaking radio burst traces back to universe's early star-forming era
Published:

In brief
Astronomers have measured the distance to the most remote fast radio burst ever recorded, FRB 20240304B, which left its source when the universe was about 3 billion years old. The James Webb Space Telescope traced the millisecond-long burst to a small, actively star-forming dwarf galaxy — not the large, mature galaxy researchers expected.
A radio signal that lasted roughly one-thousandth of a second has become the most distant fast radio burst (FRB) ever measured, according to a study published in the journal Science in October 2026. Designated FRB 20240304B, the burst traveled for more than 10 billion years before reaching Earth, originating when the universe was approximately 3 billion years old.
What was detected, and how
The burst was first picked up on March 4, 2024, by the MeerTRAP instrument on the MeerKAT radio telescope array in South Africa. Fast radio bursts are brief, intense flashes of radio waves whose physical origin is still debated; thousands have been catalogued, but only a small fraction have had their home galaxies confirmed.
To pin down how far the signal had traveled, researchers led by Manisha Caleb of the University of Sydney turned to NASA's James Webb Space Telescope. Webb's NIRCam instrument located the faint host galaxy, and its NIRSpec instrument measured the galaxy's redshift at 2.148 — the figure astronomers use to calculate cosmic distance and the age of the universe at the time light was emitted. That redshift places the burst's origin about 3 billion years after the Big Bang, during a period often called "cosmic noon," when star formation across the universe was at its peak.
The result more than doubles the distance of the previous FRB distance record, according to phys.org's report on the study.
A galaxy far smaller than expected
The host galaxy itself was the biggest surprise. Caleb and colleagues anticipated a large, well-developed galaxy, similar to many previously identified FRB hosts. Instead, Webb's images and spectra revealed a dwarf galaxy roughly 1,000 times less massive than typical FRB hosts, low in heavy elements, and in the midst of an intense burst of star formation: an estimated 90 percent of its stellar mass had formed within just the preceding 30 million years, per NASA's summary of the findings.
We thought it would be a big, nicely formed galaxy with lots of stars, and instead it was a little dwarf galaxy.
In a separate statement reported by phys.org, Caleb said the burst had been captured from a time when the universe was only about 3 billion years old, adding that researchers used that brief flash of radio light to study the matter it had traveled through over billions of years — underscoring how FRBs can be used as probes of the distant, early universe.
Why the host galaxy matters for FRB theories
Fast radio bursts have no single confirmed source. Leading explanations include magnetars — young neutron stars with extremely strong magnetic fields, typically produced by recent supernovae — and, separately, the eventual merger of two older neutron stars, a process that takes much longer to occur after a galaxy's stars form.
Because the host galaxy of FRB 20240304B is so young and still rapidly forming stars, the research team favors the magnetar explanation for this burst. NASA's account of the study notes that a young, highly magnetized neutron star could form quickly after a nearby supernova in a star-forming galaxy like this one, whereas a neutron-star merger scenario would typically require a longer delay after star formation begins.
| Property | Measurement |
|---|---|
| Burst duration | About one-thousandth of a second |
| Detection date | March 4, 2024 |
| Detection instrument | MeerKAT / MeerTRAP, South Africa |
| Redshift | 2.148 |
| Age of universe at emission | About 3 billion years |
| Travel time to Earth | Over 10 billion years |
| Host galaxy mass | About 1,000 times less massive than typical FRB hosts |
| Recent star formation | 90% of stellar mass formed in the last 30 million years |
What remains uncertain
The study identifies FRB 20240304B as the most distant FRB with a confirmed host-galaxy redshift to date, but researchers caution that a single case cannot settle the broader debate over what causes fast radio bursts. The authors note that the discovery shows little delay is required between a galaxy's star formation and its capacity to produce an FRB, but they stop short of ruling out other progenitor models for different bursts observed elsewhere in the universe.
The research team included Themiya Nanayakkara and Laura Driessen of the University of Sydney and Ben Stappers of the University of Manchester, alongside Caleb, according to NASA and phys.org accounts of the paper.
Questions
- What is FRB 20240304B?
- It is a fast radio burst — a millisecond-long flash of radio waves — detected on March 4, 2024, by the MeerKAT telescope in South Africa. It is the most distant fast radio burst with a confirmed host-galaxy distance measured so far.
- How old was the universe when the signal was emitted?
- The burst's host galaxy has a redshift of 2.148, meaning the signal left its source when the universe was about 3 billion years old, according to NASA's report on the James Webb Space Telescope measurements.
- Why is the host galaxy surprising?
- Astronomers expected a large, mature galaxy but found a dwarf galaxy roughly 1,000 times less massive than typical FRB hosts, one that was actively forming stars, with 90% of its stellar mass created in the prior 30 million years.
- What causes fast radio bursts?
- The exact cause is unconfirmed, but leading theories point to magnetars (highly magnetized young neutron stars) or mergers of older neutron stars. The young, star-forming host galaxy of this burst favors the magnetar explanation, according to the study's authors.
- Which telescopes were involved in this discovery?
- The MeerKAT radio telescope array in South Africa, using the MeerTRAP instrument, detected the burst, while NASA's James Webb Space Telescope (NIRCam and NIRSpec instruments) identified the host galaxy and measured its distance.
Sources
This piece was prepared with artificial intelligence and passed an automated source check before publication. If you see an error, ask for a correction. Request a correction or reply · How we make this
Related

SpaceArticle
How Satellites Work: Orbital Mechanics, Main Types and Everyday Uses
Satellites stay in orbit because their forward speed and Earth's gravity balance out, keeping them in continuous free fall around the planet rather than falling to the ground or flying off into space. Engineers choose an orbit's altitude, shape and inclination to match a satellite's job, from low orbits used for imaging to the geostationary belt used for weather and telecoms. As of October 2026, tracking groups count roughly 17,000 active satellites around Earth.
SpaceArticle
How Telescopes Work: Optical, Radio and Space Observatories Explained
Telescopes reveal the distant universe by collecting electromagnetic radiation — visible light, radio waves, infrared, ultraviolet, X-rays or gamma rays — and focusing it with mirrors, lenses or antenna dishes. Which design works best depends on the wavelength: ground-based optical telescopes need adaptive optics to beat atmospheric blur, radio telescopes link dishes into giant arrays, and X-ray or infrared observatories must orbit above Earth's atmosphere, which absorbs those wavelengths.
SpaceArticle
How Moon Phases Work: The Science Behind the Lunar Cycle
Moon phases are caused by the changing angle between the Sun, Earth and the Moon as the Moon orbits our planet, not by Earth's shadow. A full cycle from one new moon to the next — the synodic month — takes about 29.5 days, slightly longer than the Moon's actual 27.3‑day orbit around Earth.

SpaceGuide
How to Identify Stars and Constellations: A Beginner's Stargazing Guide
Beginners can learn to identify stars and constellations without a telescope. NASA's Night Sky Network and The Planetary Society say the naked eye is enough to start: learn a few bright anchor constellations, then use their stars as pointers to find others. Autumn and winter favor the hobby because nights are longer and, National Geographic notes, the air often offers clearer sky conditions.