Theta Ceti

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Template:Short description

Theta Ceti
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cetus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.60[2]
Characteristics
Evolutionary stage red clump[3]
Spectral type K0 III[4]
B−V Template:Engvar +1.07[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: Script error: No such module "val". mas/yr[1]
Dec.: Script error: No such module "val". mas/yr[1]
Parallax (π)29.0339±0.2198 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+0.89[6]
Details
Mass1.80[7] Template:Solar mass
RadiusScript error: No such module "val".[8] Template:Solar radius
LuminosityScript error: No such module "val".[8] Template:Solar luminosity
Surface gravity (log g)2.70[2] cgs
TemperatureScript error: No such module "val".[8] K
Metallicity [Fe/H]Script error: No such module "val".[2] dex
Rotational velocity (v sin i)2.60[2] km/s
Age2.20[7] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
θ Cet, 45 Cet, BD+08°244, FK5 47, HD 8512, HIP 6537, HR 402, SAO 129274[9]
Database references
SIMBADdata

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Theta Ceti, Latinized from θ Ceti, is a solitary,[10] orange-hued star in the equatorial constellation of Cetus. It is visible to the naked eye with an apparent visual magnitude of 3.60.[2] Based upon an annual parallax shift of 20.04 mas as seen from Earth,[1] it is located about 113 light-years from the Sun. At that distance, the visual magnitude is diminished by an extinction factor of 0.28 due to interstellar dust.[8]

With an age of about 2.2 billion years,[7] this is an evolved, K-type giant star with a stellar classification of K0 III.[4] It is a red clump[3] star on the horizontal branch,[2] which means it is generating energy through helium fusion at its core.[3] The star has an estimated 1.8[7] times the mass of the Sun and has expanded to 10 times the Sun's radius. It is radiating 58 times the solar luminosity from its photosphere at an effective temperature of 4,951 K.[8]

Name

In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Thanih al Naamat (ثاني النعامات - thānī al-naʽāmāt), which was translated into Latin as Secunda Struthionum, meaning the second ostrich.[11] This star, along with η Cet (Deneb Algenubi), τ Cet (Thalath Al Naamat), ζ Cet (Baten Kaitos) and υ Cet, were Al Naʽāmāt (النعامات), the Hen Ostriches.[12][13]

In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Square Celestial Granary, refers to an asterism consisting of θ Ceti, ι Ceti, η Ceti, ζ Ceti, τ Ceti and 57 Ceti.[14] Consequently, the Chinese name for θ Ceti itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx).[15]

References

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  13. η Cet as Aoul al Naamat or Prima Struthionum (the first ostrich), θ Cet as Thanih al Naamat or Secunda Struthionum (the second ostrich), τ Cet as Thalath al Naamat or Tertia Struthionum (the third ostrich), and ζ Cet as Rabah al Naamat or Quarta Struthionum (the fourth ostrich). υ Cet should be Khamis al Naamat or Quinta Struthionum (the fifth ostrich) consistently, but Al Achsasi Al Mouakket designated the title the fifth ostrich to γ Gam with uncleared consideration.
  14. 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.
  15. Template:In lang AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 10 日 Template:Webarchive

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Template:Stars of Cetus