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Explosion illuminates invisible galaxy in the Dark Ages

By analyzing this light, astronomers learned about a galaxy that was otherwise too small, faint, and far away for even the Hubble Space Telescope to see.
RELATED TOPICS: COSMOLOGY | GALAXIES
Gamma ray burst
This artist's illustration depicts a gamma-ray burst illuminating clouds of interstellar gas in its host galaxy. By analyzing a recent gamma-ray burst, astronomers were able to learn about the chemistry of a galaxy 12.7 billion light-years from Earth. They discovered it contains only one-tenth of the heavy elements (metals) found in our solar system. // Gemini Observatory/AURA, artwork by Lynette Cook
More than 12 billion years ago, a star exploded, ripping itself apart and blasting its remains outward in twin jets at nearly the speed of light. At its death, it glowed so brightly that it outshone its entire galaxy by a million times. This brilliant flash traveled across space for 12.7 billion years to a planet that hadn’t even existed at the time of the explosion — Earth. By analyzing this light, astronomers learned about a galaxy that was otherwise too small, faint, and far away for even the Hubble Space Telescope to see.

“This star lived at a very interesting time, the so-called Dark Ages just a billion years after the Big Bang,” said Ryan Chornock of the Harvard-Smithsonian Center for Astrophysics (CfA) in Cambridge, Massachusetts.

“In a sense, we’re forensic scientists investigating the death of a star and the life of a galaxy in the earliest phases of cosmic time.”

The star announced its death with a flash of gamma rays, an event known as a gamma-ray burst (GRB). GRB 130606A was classified as a long GRB since the burst lasted for more than four minutes. NASA’s Swift spacecraft detected it June 6. Chornock and his team quickly organized follow-up observations by the MMT Telescope in Arizona and the Gemini North Telescope in Hawaii.

“We were able to get right on target in a matter of hours,” Chornock said. “That speed was crucial in detecting and studying the afterglow.”

A GRB afterglow occurs when jets from the burst slam into surrounding gas, sweeping that material up like a snowplow, heating it, and causing it to glow. As the afterglow’s light travels through the dead star’s host galaxy, it passes through clouds of interstellar gas. Chemical elements within those clouds absorb light at certain wavelengths, leaving “fingerprints.” By splitting the light into a rainbow spectrum, astronomers can study those fingerprints and learn what gases the distant galaxy contained.

All chemical elements heavier than hydrogen, helium, and lithium had to be created by stars. As a result, those heavy elements, which astronomers collectively call “metals,” took time to accumulate. Life could not have existed in the early universe because the elements of life, including carbon and oxygen, did not exist.

Chornock and his colleagues found that the GRB galaxy contained only about one-tenth of the metals in our solar system. Theory suggests that although rocky planets might have been able to form, life probably could not thrive yet.

“At the time this star died, the universe was still getting ready for life. It didn’t have life yet, but was building the required elements,” said Chornock.

At a redshift of 5.9, or a distance of 12.7 billion light-years, GRB 130606A is one of the most distant gamma-ray bursts ever found.

“In the future, we will be able to find and exploit even more distant GRBs with the planned Giant Magellan Telescope,” said Edo Berger of the CfA.
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