Astronomers find record-old cosmic explosion

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The explosion, known as a short gamma-ray burst (GRB), took place 7.4 billion years ago, more than halfway back to the Big Bang.

"This discovery dramatically moves back the time at which we know short GRBs were exploding. The short burst is almost twice as far as the previous confirmed record holder," says John Graham, a graduate student in the Henry A. Rowland Department of Physics and Astronomy at The Johns Hopkins University. Graham is presenting his group's discovery at the American Astronomical Society's 2008 winter meeting this week in Austin, Texas.

GRBs are among the most powerful explosions in the universe, releasing enormous amounts of energy in the form of X-rays and gamma rays. Most bursts fall in one of two categories: long bursts and short bursts, depending on whether they last more or less than three seconds. Astronomers believe that long GRBs are triggered by the collapse and explosion of massive stars. In contrast, a variety of mechanisms has been proposed for short bursts. The most popular model says that most short GRBs occur when two neutron stars smash into each other and collapse into a black hole, ejecting energy in two counter-flowing beams.

The record-setting short burst is known as GRB 070714B, named because it was the second GRB detected on July 14, 2007. NASA's Swift Gamma-Ray Burst Mission discovered the GRB in the constellation Taurus. Rapid follow-up observations with the 2-meter Liverpool Telescope and the 4-meter William Herschel Telescope found an optical afterglow in the same location as the burst, which allowed astronomers to identify the GRB's host galaxy.

Next, Graham and his colleagues, Andrew Fruchter of the Space Telescope Science Institute and Andrew Levan of the University of Warwick in the United Kingdon, trained the 8-meter Gemini North Telescope in Hawaii on the galaxy. Analysis of a spectrum of the light from that galaxy indicated that it is 7.4 billion light-years away, meaning the explosion occurred 7.4 billion years ago.

"The fact that this short burst is so far away means this subclass has a broad range of distances, although they still tend to be closer on average than long GRBs," says Swift lead scientist Neil Gehrels of NASA's Goddard Space Flight Center in Greenbelt, Md.

Gehrels adds that GRB 070714B's energy was about 100 times higher than average for short bursts, more similar to the typical energy of a long GRB.

"It is unclear whether another mechanism is needed to explain this explosion, such as a neutron star-black hole merger," Gehrels said. "Or it could be that there are a wide range of energies for neutron star-neutron star mergers, but that seems unlikely."

Another possibility is that GRB 070714B concentrated its energy in two very narrow beams and that one of the beams happened to be aimed directly at Earth, making the burst seem more powerful than it really was. Researchers wonder if most short GRBs eject their energy in wider, less concentrated beams.

"We now have a good idea of the type of star that produces the brighter long bursts. But how short bursts are formed remains a mystery," Fruchter said.

Johns Hopkins University