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Before (left) and after (right) energy maps (>100 MeV) of the GRB 130427A event, as seen by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope. GRB 130427A was located in the constellation Leo, near its border with Ursa Major, at right ascension 11:32:32.90, and declination +27:41:56.5 (J2000). (Image: NASA/DOE/Fermi LAT Collaboration.) |
"GRB 130427A had the largest fluence, highest-energy photon (95 GeV), longest γ-ray duration (20 hours), and one of the largest isotropic energy releases ever observed from a GRB."[3]Low energy gamma ray bursts are observed about once per day, but GRB 130427A was an energetic exception.[9] The initial surge of gamma rays arrived at Earth at about 3:47 a.m. EDT, April 27, 2013, and it was the second brightest gamma ray burst.[6] Astronomers were prepared for such an event, and optical astronomers were immediately informed of the burster's position. A collection of optical telescopes, called the Rapid Telescopes for Optical Response (RAPTOR) Project detected a magnitude 7 brightening, which is strong enough to be observed with binoculars. The optical flash continued for 80 seconds, and there's a galaxy (SDSS J113232.84+274155.4) nearly coincident with the observed position.[4,6] A gamma ray intensity of 95 GeV was recorded at the optical peak. This is the highest intensity for a gamma ray associated with a burst. Gamma rays were detected for twenty hours, and it's estimated that the burster was at a distance of about 3.8 billion light years.[4,8] This seems like a long distance, but it's about a third the distance of similar events.[8] Energetic X-rays were observed for more than a day by another NASA space observatory, the Nuclear Spectroscopic Telescope Array (NuSTAR).[4]
![]() | Gamma ray bursts are thought to arise from particle jets, ejected at nearly light speed, from a collapsing star. (Still image from a NASA animation, via YouTube.[11]) |
"We expect to see an event like this only once or twice a century, so we're fortunate it happened when we had the appropriate collection of sensitive space telescopes with complementary capabilities available to see it."[4]Although GRB 130427A was closer to Earth than other gamma ray bursters, its radiation was easily absorbed by Earth's atmosphere. Such a burst within 1,000 light years would be another matter, since it could damage our ozone layer. However, extinction-level gamma ray bursts are expected to occur near Earth every 500 million years.[5] It's thought that the the Ordovician–Silurian extinction event, which caused the extinction of many marine species 450 million years ago, may have been caused by a nearby hypernova.[6] However, a burst comparable to GRB 130427A has a probability at less than 1 in 10 million of occurring in our galaxy.[7] The Fermi Gamma-ray Space Telescope detected thousands of gamma ray photons during its observations of GRB 130427A, but two of these were at extremely high energies. The first, at nineteen seconds into the burst, had an energy of 73 GeV. The second, at about four minutes, had an energy of 95 GeV. Not only were these energies the highest ever recorded for a gamma ray burst, they were too high in energy to be explained by the prevailing model for gamma ray bursts. Alternative models involving magnetic fields and synchrotron radiation have already been proposed.[9] It takes a lot of money to maintain such an assemblage of telescopes, and to feed 182 authors from 73 institutions. Funding in the US is from NASA and the U.S. Department of Energy.[4]