skip to content
 
Swift Science Center Italian site Italian site U.K. site U.K. site

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 have a tool dedicated to answering these questions and solving the gamma-ray burst mystery. Its three instruments give scientists the ability to scrutinize gamma-ray bursts like never before. Within seconds of detecting a burst, Swift relays its 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.

Gamma-Ray Burst With a Dual Personality

This animation illustrates two wildly different explanations for GRB 101225A, better known as the "Christmas burst." First, a solitary neutron star in our own galaxy shreds and accretes an approaching comet-like body. In the second, a neutron star is engulfed by, spirals into and merges with an evolved giant star in a distant galaxy. (Credit: NASA/Goddard Space Flight Center)
Download this video and related content from NASA Goddard's Scientific Visualization Studio

Latest Swift News
  • Swift Cycle 8 Results (22 Dec 2011)
    Swift Cycle 8 Accepted Targets and Proposals Have Been Posted
  • NASA's Swift Finds a Gamma-Ray Burst With a Dual Personality (30 Nov 2011)
    A peculiar cosmic explosion first detected by NASA's Swift observatory on Christmas Day 2010 was caused either by a novel type of supernova located billions of light-years away or an unusual collision much closer to home, within our own galaxy. Papers describing both interpretations appear in the Dec. 1 issue of the journal Nature.
  • NASA's Swift Observatory Catches Asteroid Flyby (10 Nov 2011)
    As asteroid 2005 YU55 swept past Earth in the early morning hours of Wednesday, Nov. 9, telescopes aboard NASA's Swift satellite joined professional and amateur astronomers around the globe in monitoring the fast-moving space rock. The unique ultraviolet data will aid scientists in understanding the asteroid's surface composition.
  • » Swift Newsletter
    » Signup for the Newsletter

    RSS [What is this?]

    Other News

    If you're a Swift Team member looking for the Team site, try:

    NOTE: you will need your Team username and password to access this site.


    If you have a question about Swift, please contact us via the Feedback form.

    This page was last modified on Wednesday, 14-Dec-2011 13:05:08 EST.

    NASA Astrophysics

  • Questions/Comments/Feedback
  • Find helper applications like Adobe Acrobat
  • Learn about black holes, astronomy & more!
  • A service of the Astrophysics Science Division at NASA/ GSFC

    Swift PI: Neil Gehrels,
    Responsible NASA Official: Phil Newman
    Web Curator: J.D. Myers
    PAO Contact: Francis Reddy (301-286-4453)
    Privacy Policy and Important Notices.