New ‘black neutron star’ stuns astronomers with its spectacular death

Artistic rendering of the GW190814 event, in which a smaller compact object is swallowed by a nine-times-more-massive black-hole. Alex Andrix via EGO

What happens when a star dies?

Astronomers thought they had it all figured out. A dying star either fades into a simmering white dwarf, explodes and then shrinks into a super-dense neutron star or collapses into an all-consuming black hole, depending on its mass.

However, gravitational waves detected last year suggest that a black hole may have devoured an extremely rare form of dead star — one that was heavier than a neutron star, but lighter than the lightest black hole.

Astronomers say this mystery object is the first they’ve ever seen in the “mass gap” between their definitions of neutron star and black hole. That means it might be some sort of black neutron star or to borrow the title of a Soundgarden song a black hole sun.

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Researchers detected the object’s demise last August through the U.S.-based LIGO antenna and Virgo, a similar project in Italy for monitoring the gravitational waves of huge nearby objects in space. The cosmic event sent out ripples in space-time some 780 million years ago that included hints about the mystery object’s size, according to the findings published Tuesday in the Astrophysical Journal Letters.

Scientists had suspected that objects like this one might exist, but they’d never seen one before. Now they’ll have more information to go looking elsewhere for similar objects.

“We’ve been waiting decades to solve this mystery,” study co-author Vicky Kalogera, of Northwestern University, said in a news release from LIGO. “We don’t know if this object is the heaviest known neutron star or the lightest known black hole, but either way it breaks a record.”

Stars and black holes are measured in terms of their size relative to our sun — a unit called solar mass. The largest-known neutron stars have a maximum solar mass of 2.5, while the smallest black holes start at a solar mass of five.

The mystery object had a solar mass of about 2.6, placing it in that theoretical in-between zone. It was devoured by a black hole with a solar mass of 23, and together they formed an even bigger black hole that sent invisible gravitational waves rippling toward Earth. Astronomers labelled the event “GW190814.”

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The discovery could transform scientists’ understanding of space and the way massive binary objects come together and circle one another, according to Charlie Hoy, a PhD student at Cardiff University who was part of the study.

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“We can’t rule out any possibilities,” Hoy told BBC News. “We don’t know what it is and this is why it is so exciting, because it really does change our field.”

Patrick Brady, a professor and spokesperson for the LIGO Scientific Collaboration, said the discovery should help scientists spot more of these “mass gap” objects in the future.

“The mass gap may in fact not exist at all, but may have been due to limitations in observational capabilities,” he said in the LIGO news release. “Time and more observations will tell.”

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Researchers say the event was hard to see via telescopes because the two objects would not have shone any light. The smaller object also likely wouldn’t have gone out with a bang because the black hole probably devoured it all at once.

“I think of Pac-Man eating a little dot,” Kalogera said. “When the masses are highly asymmetric, the smaller neutron star can be eaten in one bite.”

Hoy says the findings will help LIGO and Virgo scientists fine-tune their instruments so they can see more such events.

The scientists behind the discovery did not provide a new classification for the mysterious object — but whatever they eventually choose, it’ll make for a good band name in the future.

The LIGO facility first detected gravitational waves in 2016, confirming a key theoretical part of Albert Einstein’s theory of relativity. The U.S.-based LIGO and Virgo, in Italy, have detected dozens of gravitational waves since that first discovery.

Click to play video: 'Scientists discusses how proof of gravitational waves was discovered'
Scientists discusses how proof of gravitational waves was discovered

Each wave is generated by a grand cosmic event, such as the collision of two black holes or — in last year’s case — a black hole eating something that doesn’t fit into an existing category. The waves are sent out in the seconds before two huge space objects collide with one another.

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University of Chicago professor Daniel Holz, who was not part of the study, told the New York Times that the discovery is incredible because black holes and neutron stars are “polar opposites” in a sense.

“A neutron star is composed of the densest matter in the universe, and in some sense is the ultimate star,” he told the Times. “A black hole is just warped space time. It doesn’t even have a physical surface!”


Click to play video: 'Scientists confirm first direct evidence of gravitational waves'
Scientists confirm first direct evidence of gravitational waves

Holz, who is a member of the LIGO collaboration, said that in one way, black holes aren’t even part of our universe because nothing can ever escape them.

“What is astounding is that, despite their profound differences, in this particular case we can’t tell which is which,” he said.

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“Lots of theorists are now sharpening their pencils to try to explain what we’ve seen.”

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