Columba constellation is located in the southern sky. Its name means “the dove” in Latin.
Its original name was Columba Noachi, meaning “Noah’s dove,” after the dove that informed Noah that the Great Flood was receding.
The constellation was introduced by the Dutch astronomer Petrus Plancius in the late 16th century and it later appeared in Johann Bayer’s star atlas Uranometria in 1603.
Columba contains the famous runaway star Mu Columbae.
FACTS, LOCATION & MAP
Columba is the 54th constellation in size, occupying an area of 270 square degrees.
It lies in the first quadrant of the southern hemisphere (SQ1) and can be seen at latitudes between +45° and -90°.
Columba does not have any stars with known planets nor does it contain any Messier objects.
The brightest star in the constellation is Phact, Alpha Columbae.
There are no meteor showers associated with the constellation.
Columba represents Noah’s dove in the sky.
Petrus Plancius created the constellation from the stars located behind Argo Navis, the constellation that represented the Argonauts’ ship and was later split into several smaller constellations. Plancius later renamed Argo Navis to “Noah’s Ark” on a celestial globe of 1613.
In the myth, Noah’s dove is sent from the Ark to see if there is any dry land left after the Great Flood. The bird returns holding an olive branch in its beak, signalling that the flood is receding.
In some interpretations, Columba represents the dove sent by the Argonauts between the Clashing Rocks to ensure the Argonauts’ safe passage.
MAJOR STARS IN COLUMBA
Phact – α Columbae (Alpha Columbae)
Phact is the brightest star in Columba. It belongs to the spectral class B7IVe. Its name is derived from the Arabic word Al-Fakhita, which means “the dove” or “ring dove.” The star has an apparent visual magnitude of 2.60 and is approximately 270 light years distant.
Phact is a double star composed of a Be-type subgiant, a suspected Gamma Cassiopeiae type variable with an apparent magnitude varying from 2.62 to 2.66, and a faint companion star with an apparent magnitude of 12.3. The primary star has an expanding gas shell surrounding it.
Wezn – β Columbae (Beta Columbae)
Wezn (sometimes Wazn) is a giant star belonging to the spectral class K1IIICN+1. Its name comes from the Arabic word for “the weight.” It is the second brightest star in the constellation, with an apparent visual magnitude of 3.12. Wezn is approximately 86 light years distant.
Ghusn al Zaitun – δ Columbae (Delta Columbae)
Delta Columbae is a spectroscopic binary with a yellow giant for a primary component, belonging to the spectral class G7 III. It is approximately 237 light years distant and has an apparent magnitude of 3.853. Its name is derived from the Arabic phrase al-ghuşn al-zaitūn, which means “olive branch.” The giant star has a close companion with an orbital period of 2.38 years.
γ Columbae (Gamma Columbae)
Gamma Columbae is a blue subgiant (spectral class B2.5 IV) with an apparent visual magnitude of 4.35. It is located about 854 light years from the solar system.
μ Columbae (Mu Columbae)
Mu Columbae is a runaway star, believed to have been expelled from the Iota Orionis system in the Trapezium Cluster in Orion constellation. It is a fast rotating star that completes a full revolution every 1.5 days, belonging to the spectral class O9.5 V. It is one of the rare O-class stars that can be seen with the naked eye. Mu Columbae is approximately 1,300 light years distant and has an apparent magnitude of 5.15.
ε Columbae – Epsilon Columbae
Epsilon Columbae is a giant star belonging to the spectral class K1 IIIa. It is approximately 531 light years distant and has an apparent magnitude of 3.875.
η Columbae – Eta Culumbae
Eta Columbae is a yellow-orange giant (spectral type K0 III), 531.2 light years from Earth. It has an apparent magnitude of 3.946.
DEEP SKY OBJECTS IN COLUMBA
NGC 1808 is a Seyfert galaxy approximately 40 million light years distant. It is a barred spiral galaxy that shares a number of similarities with the Milky Way Galaxy. It has an unusual nucleus, shaped like a warped disk, and shows odd flows of hydrogen gas flowing out of the central regions. The galaxy is believed to have a lot of star forming activity occurring in it. A supernova was observed in the galaxy in 1993.
NGC 1851 (Caldwell 73) is a globular cluster in Columba. It has an apparent magnitude of 7.3 and is approximately 39,500 light years distant.