Iota Ceti

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Template:Short description

Iota Ceti
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cetus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.562[2]
Characteristics
Spectral type K1.5 III[3] or K1 II + (K)[4]
U−B Template:Engvar +1.278[2]
B−V Template:Engvar +1.212[2]
Variable type Suspected[5]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[6] km/s
Proper motion (μ) RA: Script error: No such module "val". mas/yr[1]
Dec.: Template:Dec mas/yr[1]
Parallax (π)11.6996±0.1968 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−1.2[7]
Details[8]
MassScript error: No such module "val". Template:Solar mass
RadiusScript error: No such module "val". Template:Solar radius
LuminosityScript error: No such module "val". Template:Solar luminosity
Surface gravity (log g)2.1[6] cgs
TemperatureScript error: No such module "val". K
Metallicity [Fe/H]−0.09[6] dex
Rotational velocity (v sin i)0.4[6] km/s
AgeScript error: No such module "val". Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
ι Cet, 8 Cet, BD−09°48, FK5 9, HD 1522, HIP 1562, HR 74, SAO 128694.[9]
Database references
SIMBADdata

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Iota Ceti (ι Cet, ι Ceti) is the Bayer designation for a star system in the equatorial constellation of Cetus. It has the traditional name Deneb Kaitos Shemali.[10] The name was from the Arabic word ذنب قيطس الشمالي - dhanab qayṭas al-shamālī, meaning the northern tail of the sea monster. it is visible to the naked eye with an apparent visual magnitude of 3.562.[2] Based upon an annual parallax shift of 11.7 mas,[11] it lies around 280 light years from the Sun.

In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Square Celestial Granary, refers to an asterism consisting of ι Ceti, η Ceti, θ Ceti, ζ Ceti, τ Ceti and 57 Ceti.[12] Consequently, the Chinese name for ι Ceti itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.)[13]

This is an MK-standard star with a stellar classification of K1.5 III,[14] indicating that it is an evolved K-type giant star. However, Houk and Swift (1999) list a classification of K1 II,[4] which would indicate this is a bright giant. It is a suspected variable with a visual amplitude of around 0.05 magnitude.[5] The star has about 3.7 times the mass of the Sun, 30 times the Sun's radius, and radiates 380 times the solar luminosity from its outer atmosphere at an effective temperature of 4,645 K.[8]

Iota Ceti forms a wide astrometric pair with a common proper motion companion,[15] a magnitude 10.40 star at an angular separation of 106.4 arcseconds along a position angle of 191° (as of 2014).[16] This companion may be a K-type star.[4]

References

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  5. a b Script error: No such module "citation/CS1". See p. 97.
  6. a b c d Script error: No such module "citation/CS1".
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  8. a b Template:Ciation
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  10. Script error: No such module "citation/CS1".
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  12. 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.
  13. Template:In lang 香港太空館 - 研究資源 - 亮星中英對照表 Template:Webarchive, Hong Kong Space Museum. Accessed on line November 23, 2010.
  14. Script error: No such module "citation/CS1".
  15. Script error: No such module "citation/CS1".
  16. Script error: No such module "citation/CS1".

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Template:Stars of Cetus Template:Sky