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Lambda Columbae information


λ Columbae

A light curve for Lambda Columbae, plotted from TESS data.[1] The 0.64 day period is marked in red.
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Columba
Right ascension 05h 53m 06.88101s[2]
Declination −33° 48′ 04.9079″[2]
Apparent magnitude (V) 4.86[3]
Characteristics
Spectral type B5 V[4]
U−B color index −0.57[3]
B−V color index −0.15[3]
Variable type Suspected rotating ellipsoidal[5]
Astrometry
Radial velocity (Rv)+30.0[6] km/s
Proper motion (μ) RA: −4.72[2] mas/yr
Dec.: +31.32[2] mas/yr
Parallax (π)9.75 ± 0.21 mas[2]
Distance335 ± 7 ly
(103 ± 2 pc)
Absolute magnitude (MV)−0.17[7]
Details
Mass4.0±0.1[4] M
Radius3.4[8] R
Luminosity213[9] L
Surface gravity (log g)4.22[10] cgs
Temperature13,524[9] K
Metallicity [Fe/H]−0.06[10] dex
Rotational velocity (v sin i)88[11] km/s
Age56.6±26.1[4] Myr
Other designations
λ Col, CD−33° 2599, HD 39764, HIP 27810, HR 2056, SAO 196276.[12]
Database references
SIMBADdata

Lambda Columbae, Latinized from λ Columbae, is a probable binary star[13] in the southern constellation of Columba. With an apparent visual magnitude of 4.86,[3] it is faintly visible to the naked eye. The measured annual parallax shift of 9.75 mas[2] yields an estimated distance of roughly 335 light years.

Lambda Columbae has a stellar classification of B5 V,[4] indicating that it is a B-type main sequence star. It is a suspected rotating ellipsoidal variable[14] with a period of 0.64 days and an amplitude of 0.07 magnitude.[15] Confirmation would indicate that this is a close binary system.[5] It has an estimated age of around 57 million years.[4]

In Chinese, (), meaning Son, refers to an asterism consisting of λ Columbae and β Columbae.[16] Consequently, λ Columbae itself is known as 子一 (Zǐ yī, English: the First Star of Son.).[17] From this Chinese name, the name Tsze is derived.[18]

  1. ^ Cite error: The named reference MAST was invoked but never defined (see the help page).
  2. ^ a b c d e f Cite error: The named reference vanLeeuwen2007 was invoked but never defined (see the help page).
  3. ^ a b c d Cite error: The named reference Mermilliod1986 was invoked but never defined (see the help page).
  4. ^ a b c d e Cite error: The named reference Tetzlaff2011 was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference Samus2012 was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference Wilson1953 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference cadars2001 was invoked but never defined (see the help page).
  9. ^ a b Cite error: The named reference Mcdonald2012 was invoked but never defined (see the help page).
  10. ^ a b Cite error: The named reference Hempel2003 was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference uesugi_fukuda1970 was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  13. ^ Cite error: The named reference Eggleton2008 was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference Morris1985 was invoked but never defined (see the help page).
  15. ^ Cite error: The named reference Hoffleit1996 was invoked but never defined (see the help page).
  16. ^ (in 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.
  17. ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 16 日
  18. ^ Cite error: The named reference Allen1963 was invoked but never defined (see the help page).

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Lambda Columbae

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Lambda Columbae, Latinized from λ Columbae, is a probable binary star in the southern constellation of Columba. With an apparent visual magnitude of 4...

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Beta Columbae

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Son, refers to an asterism consisting of Beta Columbae and Lambda Columbae. Consequently, Beta Columbae itself is known as 子二 (Zǐ èr, English: the Second...

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Ziyi

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Cyprus between Limassol and Larnaca Zi Yi (子一), a star also called Lambda Columbae Sima Liang (227–291), known as Ziyi (子翼), a regent during the Jin Dynasty...

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system 3.12 Beta Columbae Star 3.13 Delta Herculis Binary star system 3.139 3.12 HR 3803 Star 3.14 3.12 Alpha Lyncis Star 3.14 Lambda Centauri Star 3.14...

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mythology. /ᵻˈlɛktrə/ Virgo φ Virginis A Elgafar /ˈɛlɡəfɑːr/ Columba θ Columbae Elkurud /ˈɛlkərʌd/ Taurus β Tauri Aa Elnath Variously El Nath or Alnath...

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Star system

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a multiple system. This event is credited with ejecting AE Aurigae, Mu Columbae and 53 Arietis at above 200 km·s−1 and has been traced to the Trapezium...

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List of Arabic star names

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Arabic name Scientific star name Phact (al-)Fākhitah the Dove فاخثة Alpha Columbae Phad (al-)Fakhidh the Thigh فخذ Gamma Ursae Majoris Pherkad (al-)Farqad...

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Canis Major

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stars, with 3 Canis Majoris being placed by Lacaille into Columba as Delta Columbae (Flamsteed had not recognised Columba as a distinct constellation). He...

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8±0.3 A7 III or A7 IV+(n) 5.16+0.71 −0.96 2.1 3.03 (3.02 – 3.07) Beta Columbae (Wazn) 87.2±0.3 K1III_CN+1 11.5 1.1 ± 0.2 3.105 Gacrux 88.6±0.4 M3.5III...

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OB1 of Orion complex 18 1,260 4.07 combined 35,000 spectroscopy SIMBAD μ Columbae Runaway star from Trapezium Cluster 16 1,300 5.18 33,000 spectroscopy SIMBAD...

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Aviadenovirus anseris Aviadenovirus bubonis Aviadenovirus cairinae Aviadenovirus columbae Aviadenovirus columbidae Aviadenovirus falconis Aviadenovirus gallinae...

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List of Chinese star names

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Kōng Master of Constructions Beta Ceti Diphda Cetus 屎 Shǐ Excrement Mu Columbae Columba A single-star asterism in the Three Stars mansion. 郎將 Láng Jiāng...

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List of most luminous stars

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ISSN 0004-6361. S2CID 15874925. Murdin, P.; Penston, M. V. (1977-12-01). "The Lambda Orionis association". Monthly Notices of the Royal Astronomical Society...

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Stellar kinematics

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related set of runaway stars is the case of AE Aurigae, 53 Arietis and Mu Columbae, all of which are moving away from each other at velocities of over 100 km/s...

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Slow irregular variable

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Telescopium   6m.6 7m.4 0.8 M3 Iab Lc   45 G. Volantis Volans 5m.89 5m.90 0.01 M1III Lb AF Columbae Columba Perryman et al., 1997 5m.60 5m.71 0.11 M2 II/III Lb...

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