Around 12.7 billion years ago the star exploded, ripping itself apart and blasting its remains outward in twin jets at nearly the speed of light, researchers said.
At its death it glowed so brightly that it outshone its entire galaxy by a million times. This brilliant flash travelled across space for 12.7 billion years to a planet that hadn't even existed at the time of the explosion - our Earth.
By analysing this light, astronomers learned about a galaxy that was otherwise too small, faint and far away for even the Hubble Space Telescope to see.
"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," he added.
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.
It was detected by NASA's Swift spacecraft on June 6.
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.
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," says 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.
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