Above: A satellite produced image shows a flash of light produced inside a dying star just before it explodes. Scientists have for the first time witnessed the flash of light produced inside a dying star just before it explodes, according to a study on Thursday that provides a unique glimpse into how a supernova forms.
REUTERS/Kevin Schawinski (Oxford), NASA/GALEX/HST, COSMOS/Hanodut
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Scientists have for the first time witnessed the flash of light produced inside a dying star just before it explodes, according to a study on Thursday that provides a unique glimpse into how a supernova forms.
The red supergiant, more than 500 times more massive than the Earth's own sun, was destroyed after its core collapsed and a deadly shock wave of energy completely blew it up, the astronomers said.
Until now, scientists have only been able to observe the afterglow of such bursts that light up galaxies without knowing which star actually exploded, the researchers reported in the journal Science.
"We have witnessed the violent death of a massive star in a galaxy almost one billion light years away in unprecedented detail," Kevin Schawinski, an astronomer at the University of Oxford who led the study, said in a telephone interview.
"We caught the star while the supernova shock wave approached the surface of the star and then blew it apart."
A light year is the distance light travels in a year.
The researchers used images from a satellite pointed to where telescopes on Earth had detected supernovae -- which are created by the explosion of a star. They expected a first flash from inside a dying star to only be visible in ultraviolet light from space.
After the satellite produced images of a seven-hour flash, the researchers sifted through data taken from telescopes in Hawaii fixed to the same coordinates that later confirmed a supernova formed in that precise location, said Stephen Justham, a University of Oxford astronomer who worked on the study.
"The flash began just hours before the star was disrupted," he said. "How the shock wave travels in a star tells us the size of the star and what the inside is like in its final moments. The longer the flash, the bigger the star."
Understanding what happens inside a star is important because the core normally acts as a powerful nuclear furnace producing heat and pressure that makes the star shine and remain stable for a long time, the researchers said.
When the cores of these big stars run out of fuel, they collapse and spark a shock wave that travels to the surface at 20 million miles per hour to create a fireball one billion times brighter than the sun.
Supernovae are hurtling fields of heavy material that spew nickel, gold and iron, so understanding more about them can also provide insight into the formation of Earth, they added.
The Earth's sun is smaller so when it reaches the end of its life in about 4 billion years it will bloat and then shed its outer layers, leaving the remains to cool over a long period of time.
"Most of the heavy elements on Earth were made up from the inside of stars," Schawinski said. "If there hadn't been supernovae that created all these heavy elements in the distant past before the sun was formed there wouldn't have been the raw materials to form earth."
Source: Reuters
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