A Derry man has headed a team of astronomers at Queen’s University who have shed new light on the rarest and brightest exploding stars ever discovered in the universe.
Matt Nicholl.
The research has been published in Nature Magazine – one of the world’s most prestigious science publications. It proposes the most luminous supernovae – exploding stars – are powered by small and incredibly dense neutron stars, with gigantic magnetic fields that spin hundreds of times a second.
Lead author of the study is Waterside man Matt Nicholl, a former pupil of Oakgrove Integrated Primary School and Foyle College.
A research student at the Astrophysics Research Centre at Queen’s School ofMathematics and Physics he headed a team of scientists at Queen’s Astrophysics Research Centre who observed two super-luminous supernovae – two of the Universe’s brightest exploding stars – for more than a year.
Contrary to existing theories, which suggested the brightest supernovae were caused by super-massive stars exploding, their findings suggest their origins may be better explained by a type of explosion within the star’s core which creates a smaller but extremely dense and rapidly spinning magnetic star.
Matt said: “Supernovae are several billions of times brighter than the Sun, and in fact are so bright that amateur astronomers regularly search for new ones in nearby galaxies. It has been known for decades that the heat and light from these supernovae come from powerful blast-waves and radioactive material.
“But recently some very unusual supernovae have been found, which are too bright to be explained in this way. They are hundreds of times brighter than those found over the last fifty years and the origin of their extreme properties is quite mysterious.
“Some theoretical physicists predicted these types of explosions came from the biggest stars in the universe destroying themselves in a manner quite like a giant thermonuclear bomb. But our data doesn’t match up with this theory.
“In a supernova explosion, the star’s outer layers are violently ejected, while its core collapses to form an extremely dense neutron star – weighing as much as the Sun but only tens of kilometers across.
“We think that, in a small number of cases, the neutron star has a very strong magnetic field, and spins incredibly quickly – about 300 times a second. As it slows down, it could transmit the spin energy into the supernova, via magnetism, making it much brighter than normal. The data we have seems to match that prediction almost exactly.”
Queen’s astronomers led an international team of scientists on the study, using some of the world’s most powerful telescopes. Much of the data was collected using Pan-STARRS – the Panoramic Survey Telescope and Rapid Response System.
Based on Mount Haleakala in Hawaii, Pan-STARRS boasts the world’s largest digital camera, and can cover an area 40 times the size of the full moon in one shot.
The study is one of the projects funded by a prestigious €2.3million grant from the European Research Council. The grant was awarded to Professor Stephen Smartt, Director of Queen’s Astrophysics Research Centre, in 2012 to lead an international study to hunt for the Universe’s earliest supernovae.
The full article is available on Nature magazine’s website at www.nature.com/nature/journal/v502/n7471/full/nature12569.html
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