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Astronomers Simply Noticed a Gamma-Ray Explosion Defy All Recognized Space Logic : ScienceAlert

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An enormous explosion that lit up the sky did not simply rock the cosmos – it completely rattled our understanding of the Universe’s strongest outbursts.

The gamma-ray burst (GRB) recorded on 2 July 2025 is the longest of its type ever noticed, lasting a couple of day. By comparability, GRBs usually final on the size of milliseconds to minutes at most.

Moreover, it did one thing astronomers have by no means seen a GRB do earlier than: it seems to have repeated. This cannot be neatly defined by our present fashions for what causes them.

Related: Brightest Space Explosion Ever May Hide an Elusive Dark Matter Particle

“This event is unlike any other seen in 50 years of GRB observations,” says astrophysicist Antonio Martin-Carrillo of University College Dublin.

“GRBs are catastrophic events so they are expected to go off just once because the source that produced them does not survive the dramatic explosion. This event baffled us not only because it showed repeated powerful activity but also because it seemed to be periodic, which has never been seen before.”

This reddish blob is a gamma-ray burst considered billions of light-years away, repeating over the course of a day. (ESO/A. Levan, A. Martin-Carrillo et al.)

GRBs are the Universe’s most violent explosions, highly effective eruptions that blaze with probably the most energetic type of radiation – gamma rays. Each burst releases more energy in a few seconds than the Sun will over your entire course of its lifespan.

There are considered two essential mechanisms behind them: First, a core-collapse supernova of an enormous star, whereby the stellar core collapses underneath gravity to kind a black gap. This produces what we name long-duration bursts, lasting greater than two seconds.

The second mechanism includes two neutron stars colliding and merging. This produces bursts shorter than two seconds.

The uncommon nature of this new detection, designated GRB 250702B, was apparent instantly. It was found from alerts delivered by NASA’s space-based Fermi gamma-ray telescope – not simply as soon as, however three separate instances over the course of a number of hours as the thing appeared to pulsate in a number of repeated bursts of gamma rays.

The analysis group, co-led by Martin-Carrillo and astrophysicist Andrew Levan of Radboud University within the Netherlands, scurried to resolve this absolute area oddity.

A sequence of photos taken utilizing the VLT and Hubble displaying the evolution of the GRB. (ESO/A. Levan, A. Martin-Carrillo et al./NASA/ESA)

Checking different telescope information revealed that the Einstein Probe, a space-based X-ray observatory, confirmed the identical supply had been sending out X-rays nearly a full day earlier than the Fermi observations.

It was so brilliant that astronomers initially thought that the supply was proper right here within the Milky Way. However, once they educated the Very Large Telescope and the Hubble Space Telescope to the spot within the sky the place it got here from, they found in any other case.

It’s unclear precisely how far-off it’s, however the progenitor of the bizarre occasion can also be bizarre: a galaxy with a really unusual form, showing to be break up into two distinct areas. This may very well be a clue about what produced the explosions, however for the time being it is nonetheless one heck of a thriller.

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“If an enormous star – about 40 instances the mass of the Sun – had died, like in typical GRBs, then it needed to be a particular sort of demise the place some materials stored powering the central engine. Alternatively, the periodicity of the flashes of gamma-ray radiation may very well be brought on by a star being ripped aside by a black gap, a phenomenon often called a tidal disruption occasion (TDE),” Martin-Carrillo explains.

“However, not like extra typical TDEs, to elucidate the properties of this explosion would require an uncommon star being destroyed by an much more uncommon black gap, doubtless the long-sought ‘intermediate mass black gap’. Either choice could be a primary, making this occasion extraordinarily distinctive.”

To figure out what the heck GRB 250702B was, one of the first steps is to calculate the distance to the galaxy that produced it. Only then will astronomers be able to calculate its exact brightness – a measurement that will help narrow down how much energy it released, and how it may have been produced.

“We are nonetheless undecided what produced this or if we are able to ever actually discover out,” Martin-Carrillo says, “however with this analysis, we’ve got made an enormous step ahead in the direction of understanding this extraordinarily uncommon and thrilling object.”

The discovery has been detailed in The Astrophysical Journal Letters.


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