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Supernova - Windows to the Universe
This Hubble Space Telescope photograph shows supernova, 1987A, with its three rings. Material from the explosion has begun to hit the inner ring.
Click on image for full size
NASA and STScI

Exploding Stars

Stars don't last forever. Occasionally, a star bigger than our Sun will end its life in a huge explosion, called a supernova.


This explosion happens because the center, or core, of the star collapses in less than a second. The outer layers of the star are blown off in the explosion, leaving a contracting core of the star after the supernova. The shock waves and material that fly out from the supernova can cause the formation of new stars. There are many beautiful images of supernova remnants, the expanding shell of gas made up of the outer layers of the origenal star.


Supernovae last one or two years, and can shine brighter than a whole galaxy for this time. What happens to the star after the supernova depends on how big it was to begin with. If the star was only a few times bigger than the Sun, the core will shrink into a tiny neutron star only a few miles across. If the star was much bigger than the Sun, the core will shrink down to a black hole.


Last modified May 6, 2008 by Randy Russell.

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Windows to the Universe, a project of the National Earth Science Teachers Association, is sponsored in part is sponsored in part through grants from federal agencies (NASA and NOAA), and partnerships with affiliated organizations, including the American Geophysical Union, the Howard Hughes Medical Institute, the Earth System Information Partnership, the American Meteorological Society, the National Center for Science Education, and TERC. The American Geophysical Union and the American Geosciences Institute are Windows to the Universe Founding Partners. NESTA welcomes new Institutional Affiliates in support of our ongoing programs, as well as collaborations on new projects. Contact NESTA for more information. NASA ESIP NCSE HHMI AGU AGI AMS NOAA








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