The following outline is provided as an overview of and topical guide to supernovas:
A supernova (pl.: supernovae or supernovas) is a powerful and luminous explosion of a star. A supernova occurs during the last evolutionary stages of a massive star, or when a white dwarf is triggered into runaway nuclear fusion. The original object, called the progenitor, either collapses to a neutron star or black hole, or is completely destroyed to form a diffuse nebula. The peak optical luminosity of a supernova can be comparable to that of an entire galaxy before fading over several weeks or months.
What type of thing are supernovas?
editSupernovas can be described as all of the following:
Types of supernovas
editSpecific supernovas
editHistory of supernovas
editGeneral supernova concepts
editSupernova-related organizations
editSupernova-related publications
editPersons involved with supernovas
editReferences
editExternal links
edit