spaceSpace and Physics

Heavy Element Formed By Neutron Star Collision Identified For The First Time


Dr. Alfredo Carpineti

Senior Staff Writer & Space Correspondent

clockOct 23 2019, 18:00 UTC

Artist's impression of strontium being released by a neutron star collision. ESO/L. Calçada/M. Kornmesser

Turning iron into elements like gold has been a dream of alchemists for centuries, but it turns out that the true alchemists of the universe are stars. In particular, neutron star collisions, which have the ability to create elements heavier than iron.

Using gravitational waves, we have discovered a few of these collisions. The first one has been studied in detail using many telescopes and astronomers have now discovered a clear signature of strontium, an alkaline metal found in soil minerals that's used in fireworks to create red colors. As reported in Nature, strontium is also found in cosmic fireworks.


The neutron star merger GW170817 was a historic first for astronomy. The gravitational interaction was detected by the LIGO and Virgo observatories, and the subsequent kilonova explosion was seen by many optical instruments. The data continues to be examined to help us learn as much as we can about this special event.

“By reanalysing the 2017 data from the merger, we have now identified the signature of one heavy element in this fireball, strontium, proving that the collision of neutron stars creates this element in the universe,” lead author Darach Watson, from the University of Copenhagen in Denmark, said in a statement.

The process is known as "rapid neutron capture" or, more simply, r-process. Since the very first neutron star collision detection, the data has strongly shown that this process is in effect, but the complexity of neutron star collisions makes the identification of any single element difficult. At least until now.


“We actually came up with the idea that we might be seeing strontium quite quickly after the event," explained co-author Jonatan Selsing, also at the University of Copenhagen. "However, showing that this was demonstrably the case turned out to be very difficult. This difficulty was due to our highly incomplete knowledge of the spectral appearance of the heavier elements in the periodic table.” 

The r-process model was first suggested six decades ago but only now are we beginning to understand it. After the Big Bang, the universe only had hydrogen and helium (and some traces of lithium) so the rest of the elements in the periodic table had to be made by the stars.

“This is the final stage of a decades-long chase to pin down the origin of the elements,” said Watson. “We know now that the processes that created the elements happened mostly in ordinary stars, in supernova explosions, or in the outer layers of old stars. But, until now, we did not know the location of the final, undiscovered process, known as rapid neutron capture, that created the heavier elements in the periodic table.”


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