Central Engine Supernova

  • Released Wednesday, January 27, 2010
  • Updated Wednesday, November 18, 2015 at 10:52AM
  • ID: 10561

In March 2009, NASA's Swift observed the supernova SN 2009bb in the spiral galaxy NGC 3278. The explosion is apparent in visible light, but not at ultraviolet and X-ray energies, and satellites recorded no gamma-ray burst. Nevertheless, particle jets reaching 85 percent the speed of light accompanied the explosion. Astronomers believe these jets are powered by a "central engine" — likely a newborn black hole at the star's center, a scenario that also fits most gamma-ray bursts.
Supernova SN2009bb in the galaxy NGC 3278 viewed in the visible spectrum without labels.

Supernova SN2009bb in the galaxy NGC 3278 viewed in the visible spectrum without labels.

Supernova SN2009bb in the galaxy NGC 3278 viewed in the visible spectrum with labels.

Supernova SN2009bb in the galaxy NGC 3278 viewed in the visible spectrum with labels.

Supernova SN2009bb in the galaxy NGC 3278 viewed in the ultraviolet spectrum without labels.

Supernova SN2009bb in the galaxy NGC 3278 viewed in the ultraviolet spectrum without labels.

Supernova SN2009bb in the galaxy NGC 3278 viewed in the X-ray spectrum without labels.

Supernova SN2009bb in the galaxy NGC 3278 viewed in the X-ray spectrum without labels.



Credits

Please give credit for this item to:
NASA/Goddard Space Flight Center/Swift/Stefan Immler


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