Astronomers see source of gravitational waves for 1st time

A never-before-seen explosion from the merger of two dense astral bodies known as neutron stars has been viewed with telescopes for the first time.

Wave created by 2 merging neutron stars in galaxy 130 million light years from Earth

An artist's rendering of two merging neutron stars. On Aug. 17, a gravitational wave created by such an event was detected, which allowed astronomers to also witness it visually for the first time. (Robin Dienel/Carnegie Institution for Science)

A never-before-seen explosion from the merger of two dense astral bodies known as neutron stars has been viewed with telescopes for the first time.

"We did it again," National Science Foundation's director France Cordova said in a press conference on Monday.

The explosion occurred in a galaxy 130 million light years from Earth.

When these two small, but densely packed, stars merged, it triggered a cataclysmic explosion that was first seen by astronomers at the Carnegie Institution for Science's Las Campanas Observatory in northern Chile. It was followed up by 70 observatories — including the Hubble Space Telescope — and thousands of astronomers around the world.

The source brightened and then faded.

Gravitational waves are ripples in space-time, caused by highly energetic processes in space, such as the merging of black holes or neutron stars. Albert Einstein first predicted these waves in 1916 in his general theory of relativity. They remained undetected until 2015, almost 100 years later. 

While four gravitational waves have been found since the first detection in September 2015, they were the result of the merger of two black holes. And as nothing can escape a black hole, including light, there was no visible signature.

However, on Aug. 17, the Laser Interferometer Gravitational Observatory (LIGO) and Virgo experiment detected gravitational waves and determined that they were caused by two merging neutron stars that could be seen.

The astronomers at LIGO managed to roughly locate where they had originated and sent out alerts to the astronomical community in the hope that someone would also be able to visually detect them.

Maria Drout, from the Dunlap Institute for Astronomy and Astrophysics at the University of Toronto, was the first to access the telescopes in Chile in order to determine if it was possible to visually observe the source of the gravitational waves.

"It was crazy," Drout told CBC News. "It was unlike any observing nights that I've participated in."

Finding it was a nail-biting experience: astronomers had to wait 10 hours after the alerts were sent out, and even then the source would be setting on the horizon. That gave them only an hour.

It opens up a new way of observing the universe.- Harald Pfeiffer, University of Toronto

But the 10-hour wait allowed them to come up with a strategy. Once they were able to image the location, they compared them with older images taken of the same region.

And forget technology: they did it old school.

"We were looking back and forth by eye," Drout said. "We have a lot of technology to do this sort of thing now, but we really felt it was actually faster … we were literally just looking back and forth by eye to see if we saw anything new in them."

In the end, it was a colleague, Charlie Kilpatrick from the University of California, Santa Cruz, who had downloaded the image and saw the new source: a bright star-like object they named SSS17a, in galaxy named NGC 4993.

An image, right, taken Aug. 17 with the Swope Telescope at the Las Campanas Observatory in Chile shows SSS17a in the galaxy NGC 4993. The image at left, taken on April 28 with the Hubble Space Telescope shows where the neutron star merger has not occurred, and SSS17a isn't visible. (D.A. Coulter, et al.)

Turning all the telescopes they could toward the source, they tracked it for three weeks. Their observations found that it  was bright as a supernova, but the brightness decreased faster. It also became redder and cooler faster than a typical supernova.

"It's not like anything we've ever observed before," Drout said.

Answering questions

Astronomers are excited about the discovery, because it also sheds light on the creation of heavy elements like platinum and gold.

As well, it answers a 40-year-old mystery about what can cause gamma ray bursts, the most powerful form of energy in the universe.

"This time around, we have a gravitational wave from two inspiraling neutron stars, and 1.7 seconds later a gamma ray burst from the same direction in the sky," said Harald Pfeiffer, a scientist at the Canadian Institute for Theoretical Astrophysics at the University of Toronto who is part of the LIGO team, told CBC News.

NGC 4993 the source of the gravitational wave detected on Aug. 17 by the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the Virgo Interferometer. (NASA and ESA)

"So that's now confirmation that gamma ray bursts are made by colliding neutron stars."

Rainer Weiss, as well as colleagues Barry Barish and Kip Thorne, were honoured with the 2017 Nobel Prize in Physics earlier this month for their work on the discovery of the elusive waves. Hundreds of scientists around the world, including Canada, were also involved in the work.

"It's always cool discovering something really new," Pfeiffer said. "It opens up a new way of observing the universe."


Nicole Mortillaro

Senior reporter, science

Based in Toronto, Nicole covers all things science for CBC News. As an amateur astronomer, Nicole can be found looking up at the night sky appreciating the marvels of our universe. She is the editor of the Journal of the Royal Astronomical Society of Canada and the author of several books. In 2021, she won the Kavli Science Journalism Award from the American Association for the Advancement of Science for a Quirks and Quarks audio special on the history and future of Black people in science. You can send her story ideas at

With files from Emily Chung