Across the Universe, Part 2
April 29th 2009

Last year, the brightest object ever seen in the universe was detected. This was a gamma-ray burst (or GRB, in astronomers’ usual lingo) 7.5 billion light-years away, which means that the light we saw was emitted 7.5 billion years ago, more than half of the universe’s current age of 13.7 billion years.
Last week, the orbiting Swift Observatory topped that discovery with the detection of a gamma-ray burst that is 13 billion light-years away! The source of the burst is likely a supernova, the explosion of a star much more massive than our Sun. Known as Population III stars, these were the earliest stars to form in our universe, and produced the seeds of later star formation, generating chemical elements like iron, calcium, oxygen, and so forth—that are essential for life on Earth. So as far removed from daily life as this gamma-ray burst might seem, it is because such huge, early stars existed and exploded in such a violent way that we are here today.

