Stellar Collision Triggers Supernova Explosion – “This Is the First Time We’ve Actually Seen Such an Event”

Fast-Moving Debris From a Supernova Explosion

Fast-moving debris from a supernova explosion triggered by a stellar collision crashes into gas thrown out earlier, and the shocks cause bright radio emission seen by the VLA. Credit: Bill Saxton, NRAO/AUI/NSF

Astronomers have found dramatic evidence that a black hole or neutron star spiraled its way into the core of a companion star and caused that companion to explode as a supernova. The astronomers were tipped off by data from the Very Large Array Sky Survey (VLASS), a multi-year project using the National Science Foundation’s Karl G. Jansky Very Large Array (VLA).

“Theorists had predicted that this could happen, but this is the first time we’ve actually seen such an event,” said Dillon Dong, a graduate student at Caltech and lead author on a paper reporting the discovery in the journal Science.

The first clue came when the scientists examined images from VLASS, which began observations in 2017, and found an object brightly emitting radio waves but which had not appeared in an earlier VLA sky survey, called Faint Images of the Radio Sky at Twenty centimeters (FIRST). They made subsequent observations of the object, designated VT 1210+4956, using the VLA and the Keck telescope in Hawaii. They determined that the bright radio emission was coming from the outskirts of a dwarf, star-forming galaxy some 480 million light-years from Earth. They later found that an instrument aboard the International Space Station had detected a burst of X-rays coming from the object in 2014.

The data from all these observations allowed the astronomers to piece together the fascinating history of a centuries-long death dance between two massive stars. Like most stars that are much more massive than our Sun, these two were born as a binary pair, closely orbiting each other. One of them was more massive than the other and evolved through its normal, nuclear fusion-powered lifetime more quickly and exploded as a supernova, leaving behind either a black hole or a superdense neutron star.

The Sequence of Events — Clockwise, from top left: (1.) A neutron star or black hole orbits a “normal” companion star (light blue), growing closer over thousands of years. (2.) The neutron star or black hole enters its companion’s atmosphere, throwing gas outward in an expanding spiral. (3.) When the intruder reaches the companion’s core, material briefly forms a disk that propels a superfast jet outward, poking its way out of the star. The nuclear fusion that held the companion’s core up against its own gravity is disrupted, triggering a collapse and subsequent supernova explosion. (4.) The material blasted out by the supernova explosion catches up to the material thrown out by the earlier interaction, causing strong shock waves that produce the radio waves observed with the VLA. Credit: Bill Saxton, NRAO/AUI/NSF

The black hole or neutron star’s orbit grew steadily closer to its companion, and about 300 years ago it entered the companion’s atmosphere, starting the death dance. At this point, the interaction began spraying gas away from the companion into space. The ejected gas, spiraling outward, formed an expanding, donut-shaped ring, called a torus, around the pair.

Eventually, the black hole or neutron star made its way inward to the companion star’s core, disrupting the nuclear fusion producing the energy that kept the core from collapsing of its own gravity. As the core collapsed, it briefly formed a disk of material closely orbiting the intruder and propelled a jet of material outward from the disk at speeds approaching that of light, drilling its way through the star.

“That jet is what produced the X-rays seen by the MAXI instrument aboard the International Space Station, and this confirms the date of this event in 2014,” Dong said.

The collapse of the star’s core caused it to explode as a supernova, following its sibling’s earlier explosion.

“The companion star was going to explode eventually, but this merger accelerated the process,” Dong said.

The material ejected by the 2014 supernova explosion moved much faster than the material thrown off earlier from the companion star, and by the time VLASS observed the object, the supernova blast was colliding with that material, causing powerful shocks that produced the bright radio emission seen by the VLA.

“All the pieces of this puzzle fit together to tell this amazing story,” said Gregg Hallinan of Caltech. “The remnant of a star that exploded a long time ago plunged into its companion, causing it, too, to explode,” he added.

The key to the discovery, Hallinan said, was VLASS, which is imaging the entire sky visible at the VLA’s latitude — about 80 percent of the sky — three times over seven years. One of the objectives of doing VLASS that way is to discover transient objects, such as supernova explosions, that emit brightly at radio wavelengths. This supernova, caused by a stellar merger, however, was a surprise.

“Of all the things we thought we would discover with VLASS, this was not one of them,” Hallinan said.

Reference: “A transient radio source consistent with a merger-triggered core collapse supernova” 2 September 2021, Science.
DOI: 10.1126/science.abg6037 

The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.


View Comments

    • The radio images wouldn't tell you much. You need to read the paper analysis - or look at the illustrations.

  • This sort of stuff is all very interesting but it happened half a billion years ago. Is there any practical knowledge to be gained from these types of observations? Or is it just curiosity? Just asking.

    • Both. Astronomy and cosmology has a lot of applications, especially when we developed time- and position-keeping. And even if that hadn't happen, humans are curious.

  • Nothing is said about the super dense companion accreting mass as it enters the outer shells of the large normal star. With all of the gravity it has, it should get heaver and suffer significant changes to its character.

    • Systems that are organized by gravity will contract and start to interact. Take a gas cloud as illustration, when it becomes more dense swirls will average out and a net swirl will result. That's why the solar system spin, say.

National Radio Astronomy Observatory

Recent Posts

First Theorized 70 Years Ago – “Rippled Beta Sheet” Created for the First Time

University of California, Santa Cruz, scientists report the creation of three crystal structures of periodic…

October 3, 2022

Scientists Successfully Create Diamonds Out of Bottle Plastic

A research team utilizes laser flashes to replicate the interior of ice planets, which inspires…

October 3, 2022

Don’t Miss: Evenings With Giants, Mars Changes Course, and Meteors From Orion

What are some skywatching highlights in October 2022? Enjoy giant planets Jupiter and Saturn all…

October 3, 2022

Rewriting History – The First Full-Length Genomes for Homosporous Ferns

A new study reveals ferns' history of DNA hoarding and kleptomania. Ferns are infamous for…

October 3, 2022

New Research Could Change Our Understanding of Autism

Research on identifying facial emotional expressions may alter how we see autism. There is a…

October 3, 2022

Tremendous Potential – Vitamin K Found To Prevent Cell Death

Scientists discover a new function for a long-known molecule.  A team of researchers from Helmholtz…

October 3, 2022