Cosmic explosions

Kilonova

Two neutron stars collide, and the debris glows with freshly made gold

Artist's impression · drag to rotate
What it is the glow of a neutron-star merger or a neutron star meeting a black hole [1]
Powered by radioactive heavy elements made in the collision (r-process) [1]
Brightness ≈ 1 000 × a nova 1/10 to 1/100 of a typical supernova [1]
First confirmed 17 August 2017 GW170817, with the kilonova AT 2017gfo [2]
Distance ≈ 130–140 million light-years galaxy NGC 4993 [2]
Heavy elements made ≈ 16 000 × Earth's mass about 10 Earth masses of gold and platinum [2]
Colour blue, then red as the debris expanded and cooled [2]
Named 2010 Metzger et al.; first modelled in 1998 [1]

About the image. Drawn as two neutron stars just before merging, inside a red disc of debris with blue material streaming from the poles. The two colours follow how AT 2017gfo was observed; the shapes are a simplified model.

A neutron star is what is left when a massive star’s core collapses: more than a Sun’s worth of matter packed into a ball a city across. Sometimes two of them orbit each other, slowly spiralling inward as they lose energy, until they collide. The flash of light from that collision is a kilonova.

The name comes from its brightness: about a thousand times that of a classical nova, and a tenth to a hundredth of a typical supernova. Li and Paczyński described the idea in 1998, and Brian Metzger and colleagues gave it its name in 2010. For years it was only a prediction.

17 August 2017

At 12:41 UTC on 17 August 2017 the LIGO and Virgo detectors recorded a gravitational-wave signal unlike any before: not two black holes, but two lighter objects, together about 2.8 times the Sun’s mass. They were neutron stars. 1.7 seconds after the merger, NASA’s Fermi satellite caught a short gamma-ray burst from the same direction.

Within hours telescopes found a new point of light in the galaxy NGC 4993, roughly 130 to 140 million light-years away. More than 70 observatories on seven continents and in space followed it. It was the first event ever seen in both gravitational waves and light, and the kilonova, named AT 2017gfo, behaved as predicted. It started blue and turned red as the debris expanded and cooled.

Where gold comes from

The glow of a kilonova is powered by radioactivity. In the collision, neutron-rich matter is thrown out and rapidly builds up heavy atoms, a chain called the r-process. Astronomers picked out the elements strontium and yttrium in the spectrum of AT 2017gfo. In total, the merger is thought to have made heavy elements weighing about 16 000 times as much as Earth, including about ten Earth masses of gold and platinum. Collisions like this are one of the main places where the universe makes its heaviest elements.

The same event also measured gravity itself. Because the gravitational waves and the gamma rays arrived only seconds apart after travelling for over a hundred million years, the speed of gravity must equal the speed of light to within about one part in a thousand million million.

Since then

Other bursts have since been linked to mergers. GRB 211211A lasted 51 seconds, far longer than a typical short burst, yet it has been argued to come from a merger too. In 2023, GRB 230307A was associated with tellurium and other heavy elements. Each new one is a chance to watch the universe forging the atoms that end up in rings and circuit boards on Earth.

Gallery

The 3D renders come from the same model as the view at the top of this page.

Timeline

  1. 1998 Li and Paczyński describe the glow a neutron-star merger should produce.
  2. 2010 Metzger et al. name it a kilonova.
  3. 2017 GW170817 and the kilonova AT 2017gfo are seen on 17 August.
  4. 2021 GRB 211211A, a 51-second burst, is linked to a merger.
  5. 2023 GRB 230307A is associated with tellurium.

Questions people ask

Where does gold come from?

Much of it is thought to form in neutron-star collisions. The 2017 merger alone made about ten Earth masses of gold and platinum.

What is the difference between a kilonova and a supernova?

A supernova is a star exploding. A kilonova is the glow from two neutron stars colliding, and it is 10 to 100 times fainter.

How was the 2017 kilonova found?

Gravitational waves and a gamma-ray burst pointed the way, and telescopes found the new light in the galaxy NGC 4993.

Sources

  1. Wikipedia: Kilonova (Li & Paczyński 1998; Metzger et al. 2010)
  2. Wikipedia: GW170817