Alpha Columbae
α Columbae
Observation data
Epoch J2000.0 Equinox J2000.0 (ICRS) |
Constellation |
Columba |
Right ascension |
05h 39m 38.9399s[1] |
Declination |
−34° 04′ 26.788″[1] |
Apparent magnitude (V) |
2.60[1] |
Characteristics |
Spectral type |
B7IVe[1] |
U−B color index |
-0.46[2] |
B−V color index |
-0.12[2] |
R−I color index |
-0.09[2] |
Astrometry |
|
Radial velocity (Rv) |
35 ± 5[1] km/s |
Proper motion (μ) |
RA: -0.10[1] mas/yr
Dec.: -24.05[1] mas/yr |
Parallax (π) |
12.16 ± 0.60[1] mas |
Distance |
270 ± 10 ly
(82 ± 4 pc) |
Absolute magnitude (MV) |
[3] |
|
Details |
|
Mass |
4.5[4] M☉ |
Radius |
7[4] R☉ |
Luminosity (bolometric) |
1,000[4] L☉ |
Temperature |
12,500[4] K |
|
Other designations |
Alpha Columbae (α Col), CD -34°2375 , CPD -34°703, FK5 215, CSV 100672, GC 7078, HD 37795, HIP 26634, HR 1956, NSV 2549, PPM 281732, SAO 196059, CCDM J05396-3404 A. [1]
|
Database references |
SIMBAD |
data |
Alpha Columbae (α Columbae, α Col) is a 3rd magnitude and the brightest star in the constellation Columba. It is also known as Phact.
Physical charactericities
Alpha Columbae is a binary star system CCDM J05396-3404. The primary star (CCDM J05396-3404 A) is a Be-type subgiant. It is suspected Gamma Cassiopeiae type (GCAS) variable star, varying from apparent magnitude 2.62m to 2.66m. There is an expanding gas shell around the star.[5] Its faint companion (CCDM J05396-3404 B) has an apparent magnitude of 12.3m and is 13.5" distant from the primary star.[6]
Name
The proper name "Phact" (also Phad, Phaet, Phakt[5]) derived from the Arabic ألفاجتة - fākh(i)tah [fa:x(i)ta] which meaning "ring dove". It was originally applied to the constellation Cygnus as al-Fākhtah, but later transferred to this star.[7][8][9][10] The etymology of its name hadāri (unknown meaning)[11] has also been suggested.
In Chinese, 丈人 (Zhàng Rén), meaning Grandfather, refers to an asterism consisting of α Columbae and ε Columbae.[12] Consequently, α Columbae itself is known as 天囷一 (Zhàng Rén yī, English: the First Star of Grandfather.).[13] From this Chinese name, the name Chang Jin was appeared[14]
References
- ^ a b c d e f g h i * alf Col -- Be Star, database entry, SIMBAD. Accessed on line April 21, 2009.
- ^ a b c HR 1956, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line April 21, 2009.
- ^ From apparent magnitude and parallax.
- ^ a b c d Jim Kaler: Phact - STARS. Accessed on line April 21, 2009.
- ^ a b Note of HR 1956, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line April 21, 2009.
- ^ CCDM J05396-3404, database entry, J. Dommanget and O. Nys (2002) Catalogue of the Components of Double and Multiple Stars, Accessed on line April 21, 2009.
- ^ Davis, Jr., G. A., (1971). Pronunciations, Derivations, and Meanings of a Selected List of Star Names (rep. ed.). Cambridge, MA: Sky Pub. Corp. p. 11.
- ^ Kunitzsch, P., (1959). Arabische Sternnamen in Europa. Wiesbaden: Otto Harrassowitz. pp. 191–192.
- ^ Laffitte, R., (2005). Héritages arabes: Des noms arabes pour les étoiles (2éme revue et corrigée ed.). Paris: Librairie Orientaliste Paul Geunthner / Les Cahiers de l'Orient. p. 223.
- ^ Kunitzsch, P., & Smart, T., (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, MA: Sky Pub. p. 30. ISBN 978-1-931559-44-7.
- ^ Allen, R. H., (1963). Star Names: Their Lore and Meaning (rep. ed.). New York, NY: Dover Publications Inc.. p. 167. ISBN 0-486-21079-0.
- ^ (Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
- ^ (Chinese) 香港太空館 - 研究資源 - 亮星中英對照表, Hong Kong Space Museum. Accessed on line November 23, 2010.
- ^ Richard Hinckley Allen: Star Names — Their Lore and Meaning: Columbae