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Arcturus

File:Boötes_IAU.svg · Wikimedia Commons · See Wikimedia Commons

EntityQ12985· pop 79· linked from 425 articles

|- bgcolor="#FFFAFA" | Note (category: variability): || H and K emission vary.

AI overview

I don't have enough context to write an accurate 2-sentence overview. The provided information only mentions that Arcturus shows variable H and K emission, which is a technical detail insufficient for a general reader to understand what Arcturus is or why it matters.

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

~19 min read

Encyclopedic overview

13 sections
Contents
  • Nomenclature
  • Observational history
  • Observation
  • Physical characteristics
  • Spectrum
  • Oscillations
  • Search for planets
  • Mythology
  • Cultural significance
  • In popular culture
  • References
  • Further reading
  • External links

|- bgcolor="#FFFAFA" | Note (category: variability): || H and K emission vary.

Arcturus is a red giant star in the northern constellation of Boötes, and the brightest star in the constellation. It has the Bayer designation α Boötis, which is Latinized to Alpha Boötis and abbreviated Alf Boo or α Boo. With an apparent visual magnitude of −0.05, it is the fourth-brightest star in the night sky and the brightest in the northern celestial hemisphere. Arcturus forms one corner of the Spring Triangle asterism.

Excerpted from Wikipedia’s “Arcturus” article, available under the CC BY-SA 4.0 licence.

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