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Fomalhaut

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

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Also known as Alpha Piscis Austrini, 24 Piscis Austrini

Fomalhaut (, ) is the brightest star in the southern constellation of Piscis Austrinus, the Southern Fish, and one of the brightest stars in the night sky. It has the Bayer designation Alpha Piscis Austrini, which is an alternative form of α Piscis Austrini, and is abbreviated Alpha PsA or α PsA. This is a class A star on the main sequence approximately from the Sun as measured by the Hipparcos astrometry satellite. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.

AI overview

Fomalhaut is the brightest star in the constellation Piscis Austrinus and one of the brightest stars visible from Earth. Since 1943, astronomers have used its spectrum as a standard reference point for classifying other stars.

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Wikidata facts

Distance from Earth
25
Image
Wide-field view of the sky around the bright star Fomalhaut (eso1216c).jpg
Show 4 more facts
Commons category
Fomalhaut
right ascension
344.412666
declination
-29.6222222
absolute magnitude
1.72
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~16 min read

Article

11 sections
Contents
  • Nomenclature
  • Observation
  • Fomalhaut A
  • Debris disks and suspected planets
  • Fomalhaut B (TW Piscis Austrini)
  • Fomalhaut C (LP 876-10)
  • Etymology and Cultural Significance
  • See also
  • Notes
  • References
  • External links

Fomalhaut (, ) is the brightest star in the southern constellation of Piscis Austrinus, the Southern Fish, and one of the brightest stars in the night sky. It has the Bayer designation Alpha Piscis Austrini, which is an alternative form of α Piscis Austrini, and is abbreviated Alpha PsA or α PsA. This is a class A star on the main sequence approximately from the Sun as measured by the Hipparcos astrometry satellite. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.

It is classified as a Vega-like star that emits excess infrared radiation, indicating it is surrounded by a circumstellar disk.

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