Science
This
star refuses to die, even after it explodes
Swapna Krishna,Engadget
This star refuses to die,
even after it explodes
Supernovae are some of
the brightest and most energetic events in our galaxy.
These occur when stars that have much greater mass than that of our sun
explode; they become incredibly bright, and then slowly fade over the course of
a few months as they lose energy. Under the terms of how we traditionally
understand the life cycle of a star, a supernova inevitably means stellar
death. Or does it? Astronomers working at Hawaii's Keck Observatory have found
a star that refuses to die.
The supernova, named
iPTF14hls, has exploded multiple times over the last fifty years. Rather than
giving into death in the cold wastes of space, this singular star is seemingly
in a cycle of continually absorbing matter, collapsing and exploding. The team first
took note of the star in 2014 because it had gone supernova and was starting to
fade. But then, a few months later, the team noticed that the star was becoming
brighter again.
When the astronomers looked
at records, they noticed that a supernova had occurred at that same location in
1954. The star had not only somehow survived, but had gone on to explode again
in 2014. "This supernova breaks everything we thought we knew about how they work. It's the biggest puzzle I've
encountered in almost a decade of studying stellar explosions," Iair
Arcavi, the lead author of the study (which was published in Nature) said in a press release.
It's not clear why this
star refuses to die, but it could have something to do with its size. It's at
least 50 times more massive than our own star. Our conventional rules about how
stars work might not apply to something of that size. The star could also have
antimatter at its core that fuels its cycle of explosions, a hypothesized
result of its extreme mass and temperature. Regardless of the reason, we
appreciate this star's resilience
·
This
article originally appeared on Engadget.
'ZOMBIE' STAR HAS BEEN
EXPLODING FOR YEARS AND WILL NOT DIE
BY MEGHAN BARTELS ON
11/8/17
Usually, when
something explodes, that's it—it's done. That's true even in space, where stars
routinely blow themselves up. Now astronomers think they've spotted
something remarkable: a star that has exploded twice and whose current
explosion just keeps going. They reported their findings in a paper published Wednesday in the journal Nature.
Those findings are
based on studying a star that scientists had written off as not being very
interesting at first. Until, that is, an intern looked back at the data and saw
something weird. "He saw it had faded and then gotten bright again,
and that's what caught his attention," said first author Iair
Arcavi, an astronomer at the University of California, Santa
Barbara, and Las Cumbres Observatory. "That is very not normal. Supernovae
are supposed to get bright and then fade."
The aftermath of a typical, short-lived supernova as it fades. NASA'S GODDARD SPACE FLIGHT
CENTER/ESA/HUBBLE/L. CALCADA
But this one, called iPTF14hls, just kept
going and going. First spotted in September 2014, it has brightened and dimmed
five times since then, a phenomenon scientists had never seen before.
And when astronomers looked back at their
records, they found something even weirder: An explosion in exactly the same
part of the sky back in 1954. "We can't tell for sure that it's the
same star exploding," Arcavi said. "But since supernovae are so
rare and the galaxy is pretty small, we consider there's about a 95 to 99
percent chance that it's the same star."
Arcavi and his
colleagues aren't positive yet what might be happening inside the star to cause
such a weird pattern. But he pointed to a theory called pulsational pair instability as one possible
explanation. Under this scenario, a star about 100 times as large as our sun
could become so hot deep in its core that energy could turn into matter and
antimatter, which would make the star unstable.
The star would then act like
someone shoveling snow and gradually shedding outerwear: As it became
unstable, it would eject a layer of mass, which would make it stable again for
a limited time before heat builds up again. Each successive layer would
eventually collide with its predecessor, which could explain the current
pattern astronomers are seeing.
The yellow line traces the unprecedented cycle of brightening and
dimming that astronomers have watched unfold.LCO/S. WILKINSON.
But the pulsational pair instability theory
doesn't perfectly match the data Arcavi and his colleagues had gathered.
In particular, they found much more hydrogen in 2014 than they would have
expected in a star that has already exploded, since hydrogen is the lightest
element and therefore the easiest to lose.
"It's the theory that comes the closest
to explaining this," Arcavi said of pulsational pair instability.
"But it could also be something else. It could be something
completely new, which is even more exciting."
It's unusual to even be able to keep watching
a phenomenon like this every few days for three years, Arcavi added. Scientists
have only caught the iPTF14hls antics thanks to a global network of
robotic observatories that makes collecting data cheaper and easier.
Fortunately, the same technique could increase astronomers' odds of seeing
a similar event in the future—and coming one step closer to cracking the secret
of the star that just doesn't want to die.
