What is Nova?
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Overview:
Astronomers have recently performed photometric and spectroscopic observations of a recently discovered nova, known as AT 2023prq.
About Nova
- Nova is any of a class of exploding stars whose luminosity temporarily increases from several thousand to as much as 100,000 times its normal level.
- A nova reaches maximum luminosity within hours after its outburst and may shine intensely for several days or occasionally for a few weeks, after which it slowly returns to its former level of luminosity.
- Stars that become novas are nearly always too faint before eruption to be seen with the unaided eye.
- Their sudden increase in luminosity, however, is sometimes great enough to make them readily visible in the nighttime sky.
- To observers, such objects may appear to be new stars; hence the name nova, from the Latin word for “new.”
- Studying novae is crucial to advancing our knowledge about fundamental astrophysical processes, including stellar evolution.
- How do Novas occur?
- Commonly, novas start as white dwarf stars that are part of a binary star system.
- Binary stars are two stars that are close together in the distance and revolve around each other.
- The white dwarf is small and dense, and it is essentially the insides of a star that lost its outer layers. These are older stars that have lost their shine and fuel.
- The white dwarf is most likely paired with a red giant.
- The white dwarf begins to pull on its companion, the red giant, with gravitational forces.
- The white dwarf takes fuel and matter, especially hydrogen, from its companion and pulls it towards itself. The matter is quickly hurled towards the surface of the white dwarf.
- Layers of material from the red giant gather on the surface of the white dwarf. As the layers are created, the material begins to grow hotter.
- When the layers become compressed and hot enough, the material begins to combust and explodes through thermonuclear reactions.
- The hydrogen material begins to react specifically with helium. The explosion of the materials causes the white dwarf to suddenly become bright as it throws off some of the material.
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Q1) What is a Red Giant?
Red giants are stars going through their death stages. It has slowly swollen up to many times its original size. Once a star becomes a red giant, it might stay that way for up to a billion years. Then the star will slowly contract and cool to become a white dwarf. The opposite of red giants, white dwarfs are Earth-sized, ultra-dense corpses of stars radiating a tiny fraction of their original energy. Eventually, after billions of years, these stars will become totally cold and radiate no energy. They’ll end their lives as a so-called black dwarf: a tiny, burned-out, virtually-invisible cinder.
Source: Recently discovered nova investigated by astronomers