What are the causes of gamma-ray bursts? Their super-bright flashes contain clues
In July 1967, at the height of the cold war, american satellites that had been launched to search for soviet nuclear weapons tests found something totally unexpected. The Vela 3 and 4 satellites observed brief flashes of high-energy photons, or gamma rays, that appeared to be coming from space. Later, in a 1973 article that compiled more than a dozen such mysterious events, astronomers named them gamma-ray bursts. “Since then, we have tried to figure out what these explosions are,” said Andrew Taylor, a physicist at the German Electron Synchrotron (DESY) in Hamburg.
After the initial discovery, astronomers wondered where these bursts of gamma radiation came from, a vital clue as to what is fueling them. Some thought that such light sources must be nearby, in our solar system. Others have argued that they are in our galaxy, still others in the cosmos beyond. Theories abounded; the data did not.
Then, in 1997, an Italian and Dutch satellite called BeppoSAX confirmed that gamma-ray bursts were extragalactic, in some cases originating from several billion light years away.
This discovery was disconcerting. In order to account for the brightness of these objects, even when observing them from such distances, astronomers realized that the events that brought about them must be of almost unimaginable power. “We thought there was no way to get this amount of energy in an explosion from any object in the universe,” said Sylvia Zhu, astrophysicist at DESY.
A burst of gamma rays will emit the same amount of energy as a supernova, caused when a star collapses and explodes, but in seconds or minutes rather than weeks. Their maximum luminosities can be 100 trillion times that of our sun, and a billion times more than even the brightest supernovas.
Fortunately they were so far away. “If there was a gamma ray burst in our galaxy with a jet pointed at us, the best thing you can hope for is rapid extinction,” Zhu said. “You hope the radiation passes through the ozone and immediately burns everything to death. Because the worst-case scenario is if it’s further away, it could turn some of the nitrogen and oxygen in the atmosphere into nitrogen dioxide. The atmosphere would turn brown. It would be a slow death.
Gamma-ray bursts are available in two flavors, long and short. The first, which can last up to about several minutes, is said to result from stars more than 20 times the mass of our sun collapsing into black holes and exploding into supernovae. The latter, which only last about a second, are caused by the fusion of two neutron stars (or perhaps a neutron star merging with a black hole), which was confirmed in 2017 when the wave observatories gravitational have detected a fusion of NASA’s neutron and Fermi stars. The gamma-ray space telescope picked up the associated gamma-ray burst.
In each case, the gamma-ray burst does not come from the explosion itself. Rather, it is a jet moving at a fraction of the speed of light that is projected by the explosion in opposite directions. (The exact mechanism that powers the jet remains a “very basic question,” Zhu said.)
“It’s this combination of high energy speed and focus in a jet that makes them extremely bright,” said Nial Tanvir, an astronomer at the University of Leicester in England. “It means we can see them very far away.” On average, it is believed that there is an observable gamma ray burst in the visible universe every day.
Until recently, the only way to study gamma-ray bursts was to observe them from space, because the Earth’s ozone layer prevents gamma rays from reaching the surface. But when gamma rays enter our atmosphere, they collide with other particles. These particles are pushed faster than the speed of light through air, causing them to emit a blue glow known as Cherenkov radiation. Scientists can then search for these bursts of blue light.