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17/10/2013
Queen's Astronomers Shed New Light On Supernovae
Astronomers at Queen’s University have shed new light on the rarest and brightest exploding stars ever discovered in the universe, in research published today in Nature Magazine.
The research suggests that the most luminous supernovae, which are exploding stars, are powered by small neutron stars, with gigantic magnetic fields that spin hundreds of times a second.
Scientists at Queen’s Astrophysics Research Centre have contradicted existing theories with the new research.
Previous speculation suggested the supernovae are caused by super-massive stars exploding, but the new findings suggest that the origins may be explained by a type of explosion within the star’s core that creates a smaller but extremely dense and rapidly spinning magnetic star.
Matt Nicholl, a research student at the Astrophysics Research Centre at Queen’s School of Mathematics and Physics, is lead author of the study.
He 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.
It is one of the projects funded by a €2.3m 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.
He said: "These are really special supernovae. Because they are so bright, we can use them as torches in the very distant Universe. Light travels through space at a fixed speed, as we look further away, we see snapshots of the increasingly distant past. By understanding the processes that result in these dazzling explosions, we can probe the Universe as it was shortly after its birth. Our goal is to find these supernovae in the early Universe, detecting some of the first stars ever to form and watch them produce the first chemical elements created in the Universe."
(IT/CD)
The research suggests that the most luminous supernovae, which are exploding stars, are powered by small neutron stars, with gigantic magnetic fields that spin hundreds of times a second.
Scientists at Queen’s Astrophysics Research Centre have contradicted existing theories with the new research.
Previous speculation suggested the supernovae are caused by super-massive stars exploding, but the new findings suggest that the origins may be explained by a type of explosion within the star’s core that creates a smaller but extremely dense and rapidly spinning magnetic star.
Matt Nicholl, a research student at the Astrophysics Research Centre at Queen’s School of Mathematics and Physics, is lead author of the study.
He 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.
It is one of the projects funded by a €2.3m 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.
He said: "These are really special supernovae. Because they are so bright, we can use them as torches in the very distant Universe. Light travels through space at a fixed speed, as we look further away, we see snapshots of the increasingly distant past. By understanding the processes that result in these dazzling explosions, we can probe the Universe as it was shortly after its birth. Our goal is to find these supernovae in the early Universe, detecting some of the first stars ever to form and watch them produce the first chemical elements created in the Universe."
(IT/CD)
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