Gamma-ray bursts (GRBs), fleeting events that last from less than a second to several minutes, are detected by orbiting observatories that can pick up their high energy radiation. Thirteen years ago, however, astronomers discovered a longer-last…
College Park, MD (August 31, 2010) — In December 2010, IceCube — the world’s first kilometer-scale neutrino observatory, whiuch is located beneath the Antarctic ice — will finally be completed after two decades of planning. In an article in the …
Scientists “arriving quickly on the scene” of an October 4 gamma-ray burst have announced that their rapid accumulation of data has provided new insights about this exotic astrophysical phenomenon. The researchers have seen, for the first time, ongoing energizing of the burst afterglow for more than half an hour after the initial explosion. The findings support the “collapsar” model, in which the core of a star 15 times more massive than the sun collapses into a black hole. The black hole’s spin, or magnetic fields, may be acting like a slingshot, flinging material into the surrounding debris.
Scientists racing the clock have snapped a photo of a gamma-ray burst event one minute after the explosion, capturing for the first time a particularly fast-fading type of “dark” burst, which comprises about half of all gamma-ray bursts. A gamma-ray burst announces the birth of a new black hole; it is the most powerful type of explosion known, second only to the Big Bang in total energy release. This latest finding may double the number of gamma-ray bursts available for study and rattle a few theories as well, said scientists from the Massachusetts Institute of Technology, based on an X-ray image taken by the MIT-built High Energy Transient Explorer (HETE) satellite, the first satellite dedicated to spotting gamma-ray bursts.