Some of the most dramatic events in the universe are gamma-ray bursts (GRBs), brief pulses of light so bright that they can be seen from billions of light-years away. Researchers divide these events into short GRBs which last a few seconds and long GRBs which last up to a minute. For a long time, researchers thought that all long gamma-ray bursts were caused by the collapse of massive stars. But now, new research suggests that some long GRBs could be caused by two neutron stars merging.
A neutron star is the dense core that is left over after a huge star collapses, and is one of the densest objects in the universe — second only to black holes. Neutron stars have a very small size, at around 6 miles across, but hold more mass than the entire sun. So when two neutron stars collide and merge into each, the result is explosive. The merging of two neutron stars is called a kilonova, a rare event that produces a huge flash of light and is known to produce short GRBs.
But when two teams of scientists investigated a recently identified GRB which lasted for 50 seconds, putting it well into the long GRB classification, they found that it wasn’t caused by a massive star collapse but rather by a neutron star merger.
“This event looks unlike anything else we have seen before from a long gamma-ray burst,” said lead researcher Jillian Rastinejad of Northwestern University in a statement. “Its gamma rays resemble those of bursts produced by the collapse of massive stars. Given that all other confirmed neutron star mergers we have observed have been accompanied by bursts lasting less than two seconds, we had every reason to expect this 50-second GRB was created by the collapse of a massive star. This event represents an exciting paradigm shift for gamma-ray burst astronomy.”
This means that the causes of GRBs must be more complex than previously thought. If neutron star mergers can trigger both long and short GRBs, there must be something about neutron stars or GRBs which is yet to be understood.
“When you put two neutron stars together, there’s not really much mass there,” co-author Wen-fai Fong explained. “A little bit of mass accretes and then powers a very short-duration burst. In the case of massive star collapses, which traditionally power longer gamma-ray bursts, there is a longer feeding time.”
The research can also be used to help find more elusive kilonova events to study by following the trail of long GRBs as well as short ones.
“This discovery is a clear reminder that the Universe is never fully figured out,” said Rastinejad. “Astronomers often take it for granted that the origins of GRBs can be identified by how long the GRBs are, but this discovery shows us there’s still much more to understand about these amazing events.”
The research is published in the journal Nature.
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