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AT 2023prq : Nova

AT 2023prq : Nova

Astronomers have recently performed photometric and spectroscopic observations of a recently discovered nova, known as AT 2023prq.

  • 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 the 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.
  • Novas occur 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.