00h19m26s, −08° 49′26″| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Cetus |
| Right ascension | 00h19m 25.674394s[1] |
| Declination | −08° 49′ 26.10898″[1] |
| Apparent magnitude (V) | 3.562[2] |
| Characteristics | |
| Spectral type | K1.5 III[3]orK1 II + (K)[4] |
| U−B color index | +1.278[2] |
| B−V color index | +1.212[2] |
| Variable type | Suspected[5] |
| Astrometry | |
| Radial velocity (Rv) | +19.35±0.17[6] km/s |
| Proper motion (μ) | RA: −14.61 mas/yr[1] Dec.: −36.668° mas/yr[1] |
| Parallax (π) | 11.6996 ± 0.1968 mas[1] |
| Distance | 279 ± 5 ly (85 ± 1 pc) |
| Absolute magnitude (MV) | −1.2[7] |
| Details[8] | |
| Mass | 3.7±0.1 M☉ |
| Radius | 30±0.7 R☉ |
| Luminosity | 377±22 L☉ |
| Surface gravity (log g) | 2.1[6] cgs |
| Temperature | 4,645±73 K |
| Metallicity [Fe/H] | −0.09[6] dex |
| Rotational velocity (v sin i) | 0.4[6] km/s |
| Age | 230±30 Myr |
| Other designations | |
ι Cet, 8 Cet, BD−09° 48, FK5 9, HD 1522, HIP 1562, HR 74, SAO 128694.[9] | |
| Database references | |
| SIMBAD | data |
Iota Ceti (ι Cet, ι Ceti) is the Bayer designation for a star system in the equatorial constellationofCetus. 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.
InChinese, 天倉 (Tiān Cāng), 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 天倉一 (Tiān Cāng yī, English: the First Star of Square Celestial Granary.)[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]
