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

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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]]

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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.

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