Magnetic Footprints in the Glow of a Distant Explosion express

Original: "First Detection of Faraday Rotation in a Gamma-Ray Burst Afterglow: Low Polarization and High Rotation Measure in GRB 260310A Reveal Jet Magnetic Structure and Environment"
arXiv:2604.27480 · 2026-04-30 · CC BY 4.0 · 1 min
The polarization caught in the radio afterglow of a gamma-ray burst allowed astronomers to peer into the magnetic environment of the explosion.

Radio waves from a gamma-ray burst (the death of a massive star, briefly outshining its galaxy) arrive at us polarized, oscillating in a single plane, like a compass needle frozen in a magnetic field. Astronomers have read the indications of this cosmic needle for the first time.

Using spectroscopy, they traced how polarization increased with frequency: 0.7% at 11 GHz, 3.2% at 25 GHz. But even at its peak, it's far from perfect — the magnetic field in the ejected jet turned out not uniform, but made of many chaotic domains, like thousands of microscopic compasses pointing every which way.

A staggering detail: on the way to Earth, the polarization rotated by –8300 rad/m² — tens of thousands of times stronger than in our Galaxy. This Faraday rotation reveals a dense veil of ionized hydrogen around the explosion site, like a magnetic lens. Now, by tracking the dance of this needle, scientists will be able to peer into the very heart of cosmic cataclysms.

Each 'patch' of the tangled magnetic field in the jet is so tiny that from Earth it appears as a speck no larger than the Moon.

\Delta\theta = \mathrm{RM} \cdot \lambda^2
Δθ — rotation of the polarization angle, RM — rotation measure (in rad/m²), λ — wavelength (in meters)
Scientists
Michael FaradayHendrik LorentzJocelyn Bell BurnellFred HoyleAdam RiessBrian Schmidt
Concepts
afterglow rotation measure Faraday effect green bank telescope magnetar pulsations in grb xray polarization germanium detector Planck satellite gravitational wave interferometry fast radio burst 21 centimeter line fast radio telescope