Supernovae, the explosions of stars, have been observed in the thousands and in all cases they marked the death of a star.
"The spectra we obtained at Keck Observatory showed that this supernova looked like nothing we had ever seen before. This, after discovering nearly 5,000 supernovae in the last two decades," said Peter Nugent, Senior Scientist at Lawrence Berkeley National Laboratory in the US.
"While the spectra bear a resemblance to normal hydrogen-rich core-collapse supernova explosions, they grew brighter and dimmer at least five times more slowly, stretching an event which normally lasts 100 days to over two years," said Nugent.
Several months later, astronomers at Las Cumbres Observatory (LCO) in the US noticed the supernova was growing brighter again after it had faded.
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When astronomers went back and looked at archival data, they were astonished to find evidence of an explosion in 1954 at the same location. This star somehow survived that explosion and exploded again in 2014.
"This supernova breaks everything we thought we knew about how they work. It is the biggest puzzle I have encountered in almost a decade of studying stellar explosions," said Iair Arcavi, a NASA Einstein postdoctoral fellow at LCO.
Supernova iPTF14hls may have been the most massive stellar explosion ever seen, researchers said.
The size of this explosion could be the reason that our conventional understanding of the death of stars failed to explain this event, they said.
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