Death definitely becomes this star.
Astronomers reported yesterday on a massive, distant star that exploded in 2014 - and also, apparently back in 1954. This is one supernova that refuses to bite the cosmic dust, confounding scientists who thought they knew how dying stars ticked.
The oft-erupting star is 500 million light-years away - one light-year is equal to 9.5 trillion km - in the direction of the Big Bear constellation. It was discovered in 2014 and, at the time, resembled your basic supernova that was getting fainter. But a few months later, astronomers at the California-based Las Cumbres Observatory saw it getting brighter. They've seen it grow faint, then bright, then faint again five times. They've even found past evidence of an explosion 60 years earlier at the same spot.
Supernovas typically fade over 100 days. This one is still going strong after 1000 days, although it's gradually fading.
The finding was published yesterday in the journal Nature.
"It's very surprising and very exciting," said astrophysicist Iair Arcavi of the University of California, Santa Barbara, who led the study.
"We thought we've seen everything there is to see in supernovae after seeing so many of them, but you always get surprised by the universe. This one just really blew away everything we thought we understood about them."
The supernova - officially known as iPTF14hls - is believed to have once been a star up to 100 times more massive than our sun. It could well be the biggest stellar explosion ever observed, which might explain its death-defying peculiarity.
It could be multiple explosions occurring so frequently that they run into one another or perhaps a single explosion that repeatedly gets brighter and fainter, though scientists don't know how this happens.
One possibility is that this star was so massive, and its core so hot, that an explosion blew away the outer layers and left the centre intact enough to repeat the entire process. But this pulsating star theory still doesn't explain everything about this supernova, Arcavi said.
Harvard University's astronomy chairman, Avi Loeb, who was not involved in the study, speculates a black hole or magnetar - a neutron star with a strong magnetic field - might be at the centre of this never-before-seen behaviour. Further monitoring may better explain what's going on, he said.