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Bright Supernovae and Hypernovae

  • Martin Mobberley
Chapter
Part of the Astronomers' Observing Guides book series (OBSERVING)

How to observe supernovae has been covered exhaustively in the author’s book, Supernovae, and How to Observe Them. Nevertheless, when talking about the highest-energy events amateur astronomers can observe, we must include supernovae, though the subject will not be covered in as much detail here.

Supernovae mark the end state of a star’s life. In the case of a massive star the progenitor collapses into a neutron star or a black hole when it runs out of fuel. The other category of supernova involves a smaller star, but, perhaps surprisingly, an even brighter explosion. When a white dwarf star goes supernova, it is totally blown apart by a massive thermonuclear detonation (see Figure 4.1). All that is left is its companion star, which was feeding it the hydrogen that led to the explosion.

Keywords

Black Hole Neutron Star White Dwarf Solar Mass Companion Star 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Copyright information

© Springer Science+Business Media, LLC 2009

Authors and Affiliations

  • Martin Mobberley
    • 1
  1. 1.UK

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