नोवा

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

EntityQ6458· pop 70· linked from 1,374 articles

नोवा

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Also known as Bovae, Classical nova

frame|right|Artist's conception of a white dwarf, right, Accretion (astrophysics)|accreting hydrogen from the [[Roche lobe of its larger companion star]]

AI overview

A nova is a sudden, dramatic brightening of a star system caused by a thermonuclear explosion on the surface of a white dwarf that is pulling material from a nearby companion star. Novas matter to astronomers because they help us understand stellar evolution, binary star systems, and the physics of extreme conditions in space.

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

In the Vinony graph

Vinony's link graph records 1,374 inbound references to नोवा, and connects out to nebula, explosion and red giant.

Vinony files it under Astronomical events, Commons link from Wikidata and Novae.

Vinony links it to 69 Wikipedia language editions.

Wikidata facts

Instance of: astronomical phenomenon
Subclass of: variable star
Image: Making a Nova.jpg

Show 6 more facts

Commons gallery: Nova
topic's main category: Category:Novae
has list: list of novae in the Milky Way galaxy
Commons category: Novae
catalog code: N
on focus list of Wikimedia project: Wikipedia:Vital articles/Level/4

Sources (4)

via Wikidata · CC0

Gallery (12)

Categories

Astronomical events Commons link from Wikidata Novae Stellar phenomena