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File:SN1994D.jpg · Wikimedia Commons · See Wikimedia Commons

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Also known as SN, SNe, supernovae, SNO

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AI overview

A supernova is a powerful and luminous explosion of a star that occurs either during the final stages of a massive star's life or when a white dwarf undergoes runaway nuclear fusion. These explosions are so bright that their peak light can rival an entire galaxy, making them important markers for studying the universe, though the original star is either transformed into a neutron star or black hole, or destroyed entirely.

AI-generated from the Wikipedia summary — may contain errors.

Wikidata facts

Image
HST SN 1987A 20th anniversary.jpg
Show 6 more facts
topic has template
Template:Supernovae
Commons category
Supernovae
topic's main category
Category:Supernovae
model item
SN 1987A
named by
Fritz Zwicky
on focus list of Wikimedia project
Wikipedia:Vital articles/Level/4
Sources (6)

via Wikidata · CC0

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