DOE Science Showcase - Supernovae

Core collapse supernovae are extraordinary stellar explosions that mark the death throes of massive stars, with mass greater than eight to ten times the mass of the Sun.  Stars with lesser mass may also explode if they accumulate enough mass from outside to start runaway nuclear fusion.  Such explosions are the dominant source of elements in the Universe between oxygen and iron and are believed to be responsible for half of the elements heavier than iron.  They are a key link in the origin of life in the Universe. 

 

DOE researchers and their collaborators have made major advances in observing and understanding supernovae of all types.  Exciting goals are being set for future research that will be possible with improved computer representations, more precise observations and their implications and the gathering and refinement of supernovae data.  

  

See additional resources and related links about supernovae behavior and theory.

  

"The NuSTAR high-energy X-ray observatory captured this image of Cassiopeia A..."
Image Credit: Lawrence Livermore National Laboratory

 

 

Related Research Information in DOE Databases

 

 

  • DOE PAGESBeta –  journal articles and accepted manuscripts resulting from DOE funding.

 

  • SciTech Connect – reports from DOE science, technology and engineering programs. 

 

 

  • Science.gov – search results from U.S. federal science agencies. 

 

 

 

 

For additional information, see the OSTI Catalogue of Collections.

 

Additional Resources 

 

 

 Visit the Science Showcase Archive.

 

 
Last updated on Tuesday 28 April 2015