In September 2014, when astronomer Iair Arcavi discovered a brand new supernova within the night time sky, he didn’t badume a lot of it. It appeared like every other star that had simply died and violently burst aside. The object had brightened a while in the past, and now it was fading — an indication that the explosive occasion was coming to an finish. Since the juiciest half gave the impression to be over, Arcavi deserted the star looking for supernovae that had exploded extra just lately.
But robotic telescopes continued to watch the star over the following couple of months, simply in case something attention-grabbing occurred. Then, in early 2015, Arcavi requested a pupil to look by way of telescope knowledge to see if any of the celebrities they’d discovered is perhaps appearing unusual. Sure sufficient, that “ordinary” supernova wasn’t so regular anymore. It was getting brighter — nearly as if it had exploded once more. “We’ve never seen a supernova do that before,” Arcavi, an observational astronomer at UC Santa Barbara and Las Cumbres Observatory, tells The Verge.
This instantly intrigued Arcavi, so he and his staff began monitoring the star each couple days with the Las Cumbres Observatory’s telescopes situated everywhere in the world. Over the following two years, their knowledge unveiled simply how unusual the supernova was: it stayed vibrant for a prolonged 600 days, as a substitute of the everyday 100 days supernovae normally shine earlier than lastly going darkish. During this time, the star repeatedly grew brighter and fainter as much as 5 instances. It was prefer it was erupting again and again, as if the star simply refused to die.
This supernova, detailed right now within the journal Nature, is not like something ever noticed earlier than. Now, scientists are scrambling to determine what could have triggered the unusual fluctuations they noticed. The main concept is that this will have been one thing of an imposter — an occasion that appears like a supernova, however doesn’t in the end result in the destruction of a star. But even the perfect theories don’t fairly match what astronomers noticed, so the origins of this supernova nonetheless stay one thing of a thriller. “No existing model or theory of supernovae fully explains what we see here,” says Arcavi.
To study extra concerning the exploding star, the astronomers initially took its mild and separated it into its element colours, often known as taking spectra. “That allows us to get a fingerprint of the supernova,” says Arcavi. These colours can inform astronomers what supplies a star is manufactured from, how briskly it’s shifting, and the way scorching it’s. The spectra confirmed that this supernova appeared nearly precisely like the most typical supernova we find out about.
It’s additionally extremely totally different: not solely did it fluctuate in brightness for a very long time, but it surely additionally appeared to age in gradual movement, in keeping with Arcavi. Astronomers can inform how outdated a supernova is by measuring how briskly the fabric is shifting round it; normally the supplies begin to decelerate some time after a supernova has exploded. With this star, nonetheless, the supplies across the occasion remained at actually excessive speeds. So after 600 days, the supernova appeared as if it was solely 60 days outdated.
Adding to the thriller is that this star could have even exploded earlier than 2014 — truly, over half a century in the past. When digging by way of archived telescope knowledge, Arcavi and his staff discovered one other supernova that had exploded in primarily the identical spot within the sky again in 1954. They’re fairly certain it’s the identical star — or else a most unlikely coincidence. How did this star explode a minimum of as soon as within the ‘50s after which once more three years in the past?
So far, the perfect concept to clarify what’s being seen is one thing often known as pulsational pair-instability, or PPI. It’s an occasion that form of masquerades as a supernova, occurring in stars round 100 instances the mbad of our Sun. When such a star reaches the top of its life, its core can get extremely scorching — upwards of billions of levels — and turn into unstable. At this level, the oxygen contained in the core ignites and the star will blow off an outer layer of fabric. The result’s one thing that appears like a giant explosion, but it surely in the end leaves the core of the star intact. The core can then pulse like this time and again, shedding materials till it will definitely collapses right into a black gap.
No one’s ever truly seen a PPI in motion earlier than, so this could be a giant first. “It’s been in our arsenal of models for quite some time, but we’ve never had a real clincher before,” Stan Woosley, an astrophysicist who got here up with the PPI concept and wrote an accompanying article in Nature, tells The Verge. However, even the PPI concept doesn’t precisely match what Arcavi and his staff noticed. The fluctuations from a PPI are considered way more diverse in brightness, with extra time in between bursts. (Astronomers additionally didn’t badume a PPI might keep as vibrant as this occasion did for therefore lengthy.) Plus, if this star did erupt again in 1954, it in all probability would have gotten rid of most of its hydrogen again then, however Arcavi says the staff discovered the supernova to nonetheless be wealthy in hydrogen. “Maybe that model needs to be changed or revised, or this could be something completely new,” he says.
There are different much less viable explanations for the zombie star, however nothing that matches fairly proper. After a very long time shining, the supernova is now could be fading to darkness. Arcavi says his staff will proceed to watch the dimming occasion, and subsequent month NASA’s Hubble Space Telescope will observe it to presumably discover extra clues — and that’s precisely what astronomers need.
“The bottom line is we don’t know what it is, but for scientists that’s the best news of all,” says Woosley. “We love a puzzle.”