Astronomers observe the brightest flash of light EVER seen

Astronomers observe the brightest flash of light EVER seen – a 18,000,000,000,000 volt gamma-ray burst that occurred 2.4 billion light years from Earth

  • The burst of gamma-rays was first detected by orbiting telescopes on October 9
  • Its afterglow is still being watched by scientists around the world
  • The flash was recorded hitting a whopping 18,000,000,000,000 volts

Astronomers have observed the brightest flash of light ever seen –  a 18,000,000,000,000 volt burst from an event that occurred 2.4 billion light years from Earth. 

Experts believe the flash was likely triggered by the formation of a black hole.

The burst of gamma-rays – the most intense form of electromagnetic radiation – was first detected by orbiting telescopes on October 9, and its afterglow is still being watched by scientists across the world.

‘It’s really breaking records, both in the amount of photons, and the energy of the photons that are reaching us,’ said Brendan O’Connor, who used infrared instruments on the Gemini South telescope in Chile to take fresh observations early Friday.

‘Something this bright, this nearby, is really a once-in-a-century event.’

This picture provided by NASA on October 14, 2022 shows the Swift’s X-Ray Telescope capturing the afterglow of GRB 221009A about an hour after it was first detected

Gamma-ray bursts are the most violent explosions in the universe

Gamma ray bursts (GRBs), energetic jets of gamma rays that come from black holes, can be created in two different ways – resulting in long or short GRBs.

They are created from some of the most violent deaths in the Universe.

Long GRBs last about a minute, and scientists think they are produced by supernovae: when the core of a massive star collapses to become a black hole. 

Short GRBs last a second and are produced when two neutron stars merge. 

O’Connor told AFP that gamma-ray bursts that last hundreds of seconds, as occurred on Sunday, are thought to be caused by dying massive stars, greater than 30 times bigger than our Sun.

The star explodes in a supernova, collapses into a black hole, then matter forms in a disk around the black hole, falls inside, and is spewed out in a jet of energy that travels at 99.99 per cent the speed of light.

The flash released photons carrying a record 18 teraelectronvolts of energy – that’s 18 with 12 zeros behind it – and it has impacted long wave radio communications in Earth’s ionosphere.

Gamma-ray research first began in the 1960s when US satellites designed to detect whether the Soviet Union was detonating bombs in space ending up finding such bursts originating from outside the Milky Way.

‘Gamma-ray bursts in general release the same amount of energy that our Sun produces over its entire lifetime in the span of a few seconds – and this event is the brightest gamma ray burst,’ said O’Connor.

This gamma-ray burst, known as GRB 221009A, was first spotted by telescopes including NASA’s Fermi Gamma-ray Space Telescope, Neil Gehrels Swift Observatory, and Wind spacecraft on Sunday morning Eastern time.

It originated from the direction of the constellation Sagitta, and traveled an estimated 1.9 billion years to reach Earth – less than the current distance of its starting point, because the universe is expanding.

Observing the event now is like watching a 1.9 billion-year-old recording of those events unfold before us, giving astronomers a rare opportunity to glean new insights into things like black hole formation.

‘That’s what makes this sort of science so addictive – you get this adrenaline rush when these things happen,’ said O’Connor, who is affiliated with the University of Maryland and George Washington University.

Over the coming weeks, he and others will continue watching for the signatures of supernovas at optical and infrared wavelengths, to confirm that their hypothesis about the origins of the flash are correct, and that the event conforms to known physics.

Unfortunately, while the initial burst may have been visible to amateur astronomers, it has since faded out of their view.

Supernova explosions are also predicted to be responsible for producing heavy elements – such as gold, platinum, uranium – and astronomers will also be on the hunt for their signatures.

Astrophysicists have written in the past that the sheer power of gamma-ray bursts could cause extinction level events here on Earth.

But O’Connor pointed out that because the jets of energy are very tightly focused, and aren’t likely to arise in our galaxy, this scenario is not something we should worry much about.


A supernova occurs when a star explodes, shooting debris and particles into space.

A supernova burns for only a short period of time, but it can tell scientists a lot about how the universe began.

One kind of supernova has shown scientists that we live in an expanding universe, one that is growing at an ever increasing rate.

Scientists have also determined that supernovas play a key role in distributing elements throughout the universe.

In 1987, astronomers spotted a ‘titanic supernova’ in a nearby galaxy blazing with the power of over 100 million suns (pictured)

There are two known types of supernova.

The first type occurs in binary star systems when one of the two stars, a carbon-oxygen white dwarf, steals matter from its companion star.

Eventually, the white dwarf accumulates too much matter, causing the star to explode, resulting in a supernova.

The second type of supernova occurs at the end of a single star’s lifetime.

As the star runs out of nuclear fuel, some of its mass flows into its core.

Eventually, the core is so heavy it can’t stand its own gravitational force and the core collapses, resulting in another giant explosion. 

Many elements found on Earth are made in the core of stars and these elements travel on to form new stars, planets and everything else in the universe.

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