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17/10/2017
Belfast Scientist Discovers Neutron Star Smash-Up Is Source Of Gravitational Wave
A Belfast scientist from Queen's University has led an international team to a historic and ground-breaking discovery, proving that a burst of gravitational waves detected in August came from a smash up of two neutron stars.
The discovery also shows that the collision scattered gold and platinum into space.
In August, a fleet of telescopes in Chile detected a new flash of light from the same region of sky as a gravitational wave. This marked the first-ever optical detection of a gravitational wave source.
The ripples in spacetime, known as gravitational waves, are created by only the most intense moving masses as they change speed rapidly. Until August, all detected sources of gravitational waves had been black hole mergers.
Professor Stephen Smartt from the School of Maths and Physics at Queen’s University Belfast, led an international team based in Chile in scanning the sky for data. Within just 24 hours he and his team, which included Dr Kate Maguire from Queen's, were able to prove for the very first time in history that the source of the gravitational wave was the merger of two neutron stars. The research findings have been published in Nature.
The merger of the extremely dense objects, produced what is a called a kilonovae. The neutron stars are the remnants of large stars that exploded but were not massive enough to collapse into a black hole. They are extremely dense - the equivalent to the whole human race squeezed onto a teaspoon. The kilonovae have been predicted for more than 30 years but until now had never been seen.
Professor Smartt's data also shows that following the merger of the two neutron stars, a burst of rapidly expanding radioactive heavy chemical elements, including elements from caesium and tellurium all the way to gold and platinum, were scattered from the kilonova into space, moving as fast as one-fifth of the speed of light. For many years scientists had debated the origins of the elements in the periodic table that are heavier than iron and this discovery is the closest we’ve ever come to solving the mystery.
Professor Smartt said: "This discovery opens up a whole new dawn in physics and astrophysics. Einstein predicted 100 years ago that gravitational waves exist – not only have we now proved this, we have also detected the exact object that caused them – the merger of two neutron stars.
"Since the initial discovery of gravitational waves in 2016, our team at Queen’s, along with many others, have been hunting for a flash or glow in the sky that would pinpoint the exact position of gravitational waves. My team specialises in finding exploding stars and studying the highest energy events in the Universe and we were stationed at the ESO New Technology Telescope on the night that this discovery was made.
"We immediately took a spectrum at the first opportunity - a measurement that splits light up into its different components. When the spectrum appeared on our screens I realised that this was the most unusual flash in the sky that we've ever seen. I thought at that point that the merger of two neutron stars was almost certainly the source of the gravitational waves and all of our data confirmed that it was indeed the source."
The discovery also shows that the collision scattered gold and platinum into space.
In August, a fleet of telescopes in Chile detected a new flash of light from the same region of sky as a gravitational wave. This marked the first-ever optical detection of a gravitational wave source.
The ripples in spacetime, known as gravitational waves, are created by only the most intense moving masses as they change speed rapidly. Until August, all detected sources of gravitational waves had been black hole mergers.
Professor Stephen Smartt from the School of Maths and Physics at Queen’s University Belfast, led an international team based in Chile in scanning the sky for data. Within just 24 hours he and his team, which included Dr Kate Maguire from Queen's, were able to prove for the very first time in history that the source of the gravitational wave was the merger of two neutron stars. The research findings have been published in Nature.
The merger of the extremely dense objects, produced what is a called a kilonovae. The neutron stars are the remnants of large stars that exploded but were not massive enough to collapse into a black hole. They are extremely dense - the equivalent to the whole human race squeezed onto a teaspoon. The kilonovae have been predicted for more than 30 years but until now had never been seen.
Professor Smartt's data also shows that following the merger of the two neutron stars, a burst of rapidly expanding radioactive heavy chemical elements, including elements from caesium and tellurium all the way to gold and platinum, were scattered from the kilonova into space, moving as fast as one-fifth of the speed of light. For many years scientists had debated the origins of the elements in the periodic table that are heavier than iron and this discovery is the closest we’ve ever come to solving the mystery.
Professor Smartt said: "This discovery opens up a whole new dawn in physics and astrophysics. Einstein predicted 100 years ago that gravitational waves exist – not only have we now proved this, we have also detected the exact object that caused them – the merger of two neutron stars.
"Since the initial discovery of gravitational waves in 2016, our team at Queen’s, along with many others, have been hunting for a flash or glow in the sky that would pinpoint the exact position of gravitational waves. My team specialises in finding exploding stars and studying the highest energy events in the Universe and we were stationed at the ESO New Technology Telescope on the night that this discovery was made.
"We immediately took a spectrum at the first opportunity - a measurement that splits light up into its different components. When the spectrum appeared on our screens I realised that this was the most unusual flash in the sky that we've ever seen. I thought at that point that the merger of two neutron stars was almost certainly the source of the gravitational waves and all of our data confirmed that it was indeed the source."
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