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The new discovery and its spectral lines the colors of light it sent our way allowed scientists to classify it as a typical Type IIa supernova, the kind from large exploding stars. But this one remained bright for six times as long, with no sign of its ejected matter slowing down. And it sits in exactly the same spot as another supernova. All of this demonstrates just how little we know about the eventual fate of very massive stars.
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stanley cup get involved. When I saw the proofs of the paper it kind of blew my mind, Nick Konidaris, Carnegie Institution for Science astronomer, told Gizmodo. The notion that a star exploded in 1954, then left over enough material such that it could explode again, however many years later, really did not intuitively make sense to me. Robotic sky surveys spotted the new light back in September 2014, after which astronomers made repeated observations. Supernovae have a
stanley cup website lways been associated with the death of stars, according to the paper published today in Nature. And spectral lines have aways revealed these stars ejecting fast-moving matter, followed by the appearance of slower-moving matter beneath. But repeated observations of iPTF14hls didnt demonstrate this slowdown. And while other supernovae dim after 100 days, this one remained bright after over 600 days of repeated observations, including some periods where it got even brighter. On top of that, this supe
