Iota Centauri

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Template:Short description

ι Centauri
Template:Location mark
Location of ι Centauri (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) +2.73[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type A2 V[4] (kA1.5hA3mA3va)[5]
U−B Template:Engvar +0.01[2]
B−V Template:Engvar +0.03[2]
Astrometry
Radial velocity (Rv)+0.1[6] km/s
Proper motion (μ) RA: −341.11[1] mas/yr
Dec.: −86.14[1] mas/yr
Parallax (π)55.49±0.17 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+1.47[4]
Details
MassScript error: No such module "val".[7] Template:Solar mass
RadiusTemplate:Solar radius calculator[7]Template:Efn Template:Solar radius
LuminosityScript error: No such module "val".[7] Template:Solar luminosity
Surface gravity (log g)4.11[8] cgs
TemperatureScript error: No such module "val".[7] K
Metallicity [Fe/H]–0.46[8] dex
Rotational velocity (v sin i)90.3[9] km/s
Age0.35[10] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[11]
Database references
SIMBADdata

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Iota Centauri, Latinized from ι Centauri, also named Kulou,[12] is a star in the southern constellation of Centaurus. Based upon parallax measurements, it lies at a distance of approximately Script error: No such module "convert". from Earth.[1] Iota Centauri has an apparent visual magnitude of +2.73,[2] making it easily visible to the naked eye.

The spectrum of ι Centauri matches a stellar classification of A2 V. It is an A-type main sequence star that is generating energy by the nuclear fusion of hydrogen in its core region. This energy is being radiated from the outer envelope of the star at an effective temperature of 9,160 K,[7] giving the star a white hue.[13] It has about 2 times the Sun's mass, 1.9 times the Sun's radius,[7] and is roughly 350 million years old.[10] The abundance of elements other than hydrogen and helium, what astronomers term the metallicity, is only 35% of the abundance in the Sun.[8] A weak magnetic field has been tentatively identified with a strength of −77 ± 30 G.[14]

This star has an excess emission of infrared indicating it is surrounded by a circumstellar disk of dust, known as a debris disk. The disk is located within an orbital radius of six Astronomical Units from the star. The dust is unusually luminous for a star this age, suggesting that some process may have recently increased the amount of debris, such as collisions between planetesimals. Alternatively, the planetesimals in this system may have unusual physical properties. As of 2011, a search for planets in this system has thus far been unsuccessful.[10]

Iota Centauri appears to belong to the stellar kinematic group known as IC 2391. This is a group of around 16 co-moving stars that most likely originated in the same molecular cloud at least 45 million years ago.[15]

Nomenclature

In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Pillars, refers to an asterism consisting of ι Centauri, υ2 Centauri, υ1 Centauri, a Centauri, ψ Centauri, 4 Centauri, 3 Centauri and 1 Centauri.[16] Consequently, the Chinese name for ι Centauri itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.)[17]

In older Chinese sources,[18] this star was a member of the ancient super-constellation Kulou (库楼, The Arsenal), in the area of modern Centaurus and Lupus, dating back to the 2nd century BCE.[12] Later, ζ Centauri was identified as the main star of Kulou.[18] The IAU Working Group on Star Names approved the name Kulou for this star on 17 February 2025 and it is now so entered in the IAU Catalog of Star Names.[12]

Notes

Template:Notelist

References

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  14. Script error: No such module "citation/CS1".
  15. Script error: No such module "citation/CS1".
  16. Template:In lang 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, Template:ISBN.
  17. Template:In lang AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 25 日 Template:Webarchive
  18. a b Script error: No such module "citation/CS1".

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Template:Stars of Centaurus