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Columba (constellation)





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Columba is a faint constellation designated in the late sixteenth century, remaining in official use, with its rigid limits set in the 20th century. Its name is Latin for dove. It takes up 1.31% of the southern celestial hemisphere and is just south of Canis Major and Lepus.

Columba
Constellation
Columba
AbbreviationCol
GenitiveColumbae
Pronunciation/kəˈlʌmbə/,
genitive /kəˈlʌmb/
Symbolismthe dove
Right ascension05h03m 53.8665s06h39m 36.9263s[1]
Declination−27.0772038°–−43.1116486°[1]
Area270 sq. deg. (54th)
Main stars5
Bayer/Flamsteed
stars
18
Stars with planets1
Stars brighter than 3.00m1
Stars within 10.00 pc (32.62 ly)0
Brightest starα Col (Phact) (2.65m)
Messier objects0
Meteor showers0
Bordering
constellations
Lepus
Caelum
Pictor
Puppis
Canis Major
Visible at latitudes between +45° and −90°.
Best visible at 21:00 (9 p.m.) during the month of February.

History

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The constellation Columba as it can be seen by the naked eye.
 
The constellation seen as "Columba Noachi" in Urania's Mirror (1825).

In the Society Islands, Alpha Columbae (Phact) was called Ana-iva.[10]

Features

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Stars

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Columba is rather inconspicuous, the brightest star, Alpha Columbae, being only of magnitude 2.7. This, a blue-white star, has a pre-Bayer, traditional, Arabic name Phact (meaning ring dove) and is 268 light-years from Earth. The only other named star is Beta Columbae, which has the alike-status name Wazn. It is an orange-hued giant star of magnitude 3.1, 87 light-years away.[11]

The constellation contains the runaway star μ Columbae, which was probably expelled from the ι Orionis system.

Exoplanet NGTS-1b and its star NGTS-1 are in Columba.

General radial velocity

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Columba contains the solar antapex – the opposite to the net direction of the solar system[12] (noting the local spiral arm of the Milky Way itself is responsible for most of our change of position over time).[citation needed]

Deep-sky objects

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NGC 1851aglobular cluster in Columba appears at 7th magnitude in a far part of our galaxy as is 39,000 light-years away - it is resolvable south of at greatest latitude +40°N in medium-sized amateur telescopes (under good conditions).[11]

See also

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Citations

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  1. ^ a b "Columba, constellation boundary". The Constellations. International Astronomical Union. Retrieved 27 February 2014.
  • ^ B. Schildgen (2016). Heritage or Heresy: Preservation and Destruction of Religious Art and Architecture in Europe. Springer. p. 63. ISBN 978-0-230-61315-7.
  • ^ a b Ridpath & Tirion 2001, pp. 120–121.
  • ^ Ley, Willy (December 1963). "The Names of the Constellations". For Your Information. Galaxy Science Fiction. pp. 90–99.
  • ^ Canis Maior and Columba in Bayers Uranometria 1603 (Linda Hall Library) Archived 2007-04-27 at the Wayback Machine
  • ^ Richard H. Allen (1899) Star Names: Their Lore and Meaning, pp. 166–168
  • ^ P.K. Chen (2007) A Constellation Album: Stars and Mythology of the Night Sky, p. 126 (ISBN 978-1-931559-38-6).
  • ^ Chen, p. 126.
  • ^ "NASA's OSIRIS-REx Students Catch Unexpected Glimpse of Newly Discovered Black Hole". NASA. 28 February 2020.
  • ^ Makemson 1941, p. 281.
  • ^ a b Ridpath & Tirion 2017, p. 122.
  • ^ Madore, Barry F. (14 August 2002). "Astronomical Glossary". NASA/IPAC Extragalactic Database. Retrieved 31 January 2023.
  • References

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  •   Stars
  •   Spaceflight
  •   Outer space
  •   Solar System

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=Columba_(constellation)&oldid=1221595822"
     



    Last edited on 30 April 2024, at 21:06  





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    This page was last edited on 30 April 2024, at 21:06 (UTC).

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