- Scientists have detected the brightest, most energetic light in the universe for the first time: Telescopes captured two violent space explosions called gamma-ray bursts.
- Astronomers acted quickly to capture this ultra-high-energy light, turning telescopes on Earth toward the explosion just 50 seconds after NASA satellites detected it.
- The ultra-high-energy light appeared in the gamma-ray burst’s afterglow, not in the initial explosion – a fact that is giving scientists new clues about how gamma-ray bursts produce ultra-high-energy light.
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Two violent explosions in galaxies billions of light-years away recently produced the brightest light in the universe. Scientists caught it in action for the first time.
The explosions were gamma-ray bursts, short eruptions of the most energetic form of light in the universe.
Telescopes caught the first burst in July 2018. The second burst, captured in January, produced light containing about 100 billion times as much energy as the light that’s visible to our eyes.
Gamma-ray bursts appear without warning and last only a few seconds, so astronomers had to move quickly. Just 50 seconds after satellites spotted the January explosion, telescopes on Earth swiveled to catch a flood of thousands of particles of light.
“These are by far the highest-energy photons ever discovered from a gamma-ray burst,” Elisa Bernardini, a gamma-ray scientist, said in a press release on Wednesday.
Over 300 scientists around the world studied the results; their work was published on Wednesday in the journal Nature.
50 seconds to capture the brightest, most mysterious light in the universe
Gamma-ray bursts happen almost every day, without warning, and they last just a few seconds. Yet the high-energy explosions remain something of a mystery to scientists. Astronomers think they come from colliding neutron stars or from supernovae – events in which stars run out of fuel, give in to their own gravity, and collapse into black holes.
“Gamma-ray bursts are the most powerful explosions known in the universe and typically release more energy in just a few seconds than our sun during its entire lifetime,” David Berge, a gamma-ray scientist, said in the release. “They can shine through almost the entire visible universe.”
The brief, intense eruptions of gamma rays are followed by hours or days of afterglow.
Telescopes have observed low-energy rays that come from the initial explosion and the afterglow.
“Much of what we’ve learned about GRBs over the past couple of decades has come from observing their afterglows at lower energies,” Elizabeth Hays, a NASA scientist, said in a release.
But scientists had never caught the ultra-high-energy light until these two recent observations.
On January 14, two NASA satellites detected an explosion in a galaxy over 4 billion light-years away. Within 22 seconds, these space telescopes – the Neil Gehrels Swift Observatory and the Fermi Gamma-Ray Space Telescope – beamed the coordinates of the burst to astronomers all over Earth.
Within 27 seconds of receiving the coordinates, astronomers in the Canary Islands turned two Major Atmospheric Gamma Imaging Cherenkov telescopes toward that point in the sky.
The photons flooded those telescopes for the next 20 minutes, leading to new revelations about some of the most elusive properties of gamma-ray bursts.
“It turns out we were missing approximately half of their energy budget until now,” Konstancja Satalecka, a scientist who coordinates the telescopes’ searches for gamma-ray bursts, said in the release. “Our measurements show that the energy released in very-high-energy gamma-rays is comparable to the amount radiated at all lower energies taken together. That is remarkable.”
Ultra-high-energy light came in the afterglow, not the explosion itself
The photons detected from a gamma-ray burst six months earlier, in July 2018, weren’t as energetic or as numerous as those from the January explosion.
But the earlier detection was still notable because the flow of high-energy light came 10 hours after the initial explosion. The light lasted for another two hours – deep into the afterglow phase.
In their paper, the researchers suggested that electrons may have scattered the photons, increasing the photons’ energy. Another paper about the January observations suggested the same thing.
Scientists had long suspected that this scattering was one way that gamma-ray bursts could produce so much ultra-high-energy light in the afterglow phase. The observations of these two bursts confirmed that for the first time.
Scientists expect to learn more as they turn telescopes toward more gamma-ray bursts like these in the future.
“Thanks to these new ground-based detections, we’re seeing the gamma rays from gamma-ray bursts in a whole new way,” Hays said.
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