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超新星

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Also known as SN, SNe, supernovae, SNO

大質量の恒星や近接連星系の白色矮星が起こす大規模な爆発（超新星爆発）によって輝く天体

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.

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Wikidata facts

Subclass of: astronomical phenomenon
Image: HST SN 1987A 20th anniversary.jpg

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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

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Article · 日本語

超新星（ちょうしんせい、英: supernova、スーパーノヴァ）は、大質量の恒星や近接連星系の白色矮星が起こす大規模な爆発（超新星爆発）によって輝く天体のこと。

Abstract from DBpedia / Wikipedia · CC BY-SA

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