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The Swift Gamma-Ray Burst Mission

Swift satellite artists conception Gamma-ray bursts (GRBs) are the most powerful explosions the Universe has seen since the Big Bang. They occur approximately once per day and are brief, but intense, flashes of gamma radiation. They come from all different directions of the sky and last from a few milliseconds to a few hundred seconds. So far scientists do not know what causes them. Do they signal the birth of a black hole in a massive stellar explosion? Are they the product of the collision of two neutron stars? Or is it some other exotic phenomenon that causes these bursts?

With Swift, a NASA mission with international participation, scientists will now have a tool dedicated to answering these questions and solving the gamma-ray burst mystery. Its three instruments will give scientists the ability to scrutinize gamma-ray bursts like never before. Within seconds of detecting a burst, Swift will relay a burst's location to ground stations, allowing both ground-based and space-based telescopes around the world the opportunity to observe the burst's afterglow. Swift is part of NASA's medium explorer (MIDEX) program and was launched into a low-Earth orbit on a Delta 7320 rocket on November 20, 2004.

XRT and UVOT Image of GRB 080319B
XRT and UVOT Image of GRB 080319B.

+ Learn more

Latest Swift Gamma-Ray Bursts
September 15, 2008 GRB080915b

September 15, 2008 GRB080915

September 13, 2008 GRB080913

+ All Swift Bursts (Updated September 15, 2008)
+ Data Table of Swift Bursts
+ GCN Circulars Archive
+ GRB Skymap

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This page was last modified on Monday, 15-Sep-2008 13:06:20 EDT.

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