Why do novas shine?

In summary, novas shine due to the explosive nuclear fusion that occurs on the surface of a white dwarf star when it accumulates enough hydrogen from a companion star. This process causes a sudden increase in brightness, often outshining entire galaxies for a short period. The energy released during this fusion event results in the characteristic bright flash associated with a nova.
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Brzohn
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It’s my understanding that a nova happens when you have a close binary star, and one component is a white dwarf. The white dwarf sucks hydrogen from its companion, the hydrogen piles up on the surface of the dwarf until it’s hot and dense enough to undergo nuclear fusion. Ka-boom. Right?

Why is this energy visible light? Nuclear reactions produce energy in the form of gamma rays and moving particles. The reaction is on the surface of the star; the energy isn’t emitted in the middle of an atmosphere that it could be Compton scattered down the spectrum, or heat up the atmosphere till it glows. By my reasoning, a nova should emit gamma and cosmic rays, but not visible light. What’s going on?
 
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Until just about now I've had the same misconception as you, I think. That the white dwarf is essentially a naked core emitter.
Take a look at this paper:
https://articles.adsabs.harvard.edu/pdf/2012MmSAI..83..779K
There's a brief overview of the process in the introduction.

The key takeaways seem to be:
The nova white dwarf has an atmosphere accreted from its companion. It then emits light from its photosphere, much like a regular star. The photosphere expands significantly during the nova event, on the order of a hundred solar radii, giving rise to the initial luminosity spike. Subsequently, Bremsstrahlung radiation in the ejecta take over as the main contributor to the light curve.
I.e. it doesn't appear to be the case that the fusing surface is ever exposed.
 
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By the same argument, the sun should not emit visible light either. Does that point you in the right direction?
 
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FAQ: Why do novas shine?

What is a nova?

A nova is a type of astronomical event that occurs in a binary star system, where a white dwarf star accumulates material from a companion star. When enough material builds up on the surface of the white dwarf, it undergoes a thermonuclear explosion, resulting in a sudden and dramatic increase in brightness.

Why do novas shine so brightly?

How long does the brightness of a nova last?

The brightness of a nova typically lasts from a few days to several weeks, depending on the specific characteristics of the nova. After reaching its peak brightness, the nova gradually fades as the nuclear fusion process slows down and the expelled material disperses into space.

What causes the variability in nova brightness?

The variability in nova brightness can be attributed to several factors, including the amount of material that accumulates on the white dwarf, the rate of fusion reactions, and the geometry of the binary system. Each nova can have a different peak brightness and duration, influenced by these factors.

Are novas the same as supernovae?

No, novas and supernovae are distinct phenomena. A nova is a smaller-scale explosion in a binary system involving a white dwarf, while a supernova is a more powerful explosion that occurs at the end of a massive star's life cycle, resulting in the star's complete destruction. Supernovae release significantly more energy and can outshine entire galaxies for a longer duration.

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