Observation data Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation
Cetus
Right ascension
01h 51m 27.63482s[1]
Declination
−10° 20′ 06.1289″[1]
Apparent magnitude (V)
3.742[2]
Characteristics
Spectral type
K0 III Ba0.1[3]
U−B color index
+1.076[2]
B−V color index
+1.131[2]
Variable type
Suspected[4]
Astrometry
Radial velocity (Rv)
+10.86±0.64[5] km/s
Proper motion (μ)
RA: +40.80[1] mas/yr Dec.: −37.25[1] mas/yr
Parallax (π)
13.88 ± 0.57 mas[1]
Distance
235 ± 10 ly (72 ± 3 pc)
Absolute magnitude (MV)
−0.54[6]
Orbit[7]
Period (P)
1,652 d
Eccentricity (e)
0.59
Longitude of the node (Ω)
85°
Periastron epoch (T)
2414377 JD
Semi-amplitude (K1) (primary)
3.3 km/s
Details[5]
ζ Cet A
Mass
2.34[8]M☉
Radius
25 R☉
Luminosity
240 L☉
Surface gravity (log g)
2.4 cgs
Temperature
4,581±14 K
Metallicity [Fe/H]
−0.13 dex
Rotational velocity (v sin i)
3.2 km/s
Age
1.24[8] Gyr
Other designations
Baten Kaitos, ζ Cet, 55 Cet, BD−11°359, FK5 62, HD 11353, HIP 8645, HR 539, SAO 148059, WDS J01515-1020A.[9]
Database references
SIMBAD
data
Zeta Ceti (ζ Ceti, abbreviated Zeta Cet, ζ Cet) is a binary star in the equatorial constellation of Cetus. It has a combined apparent visual magnitude of 3.74,[2] which is bright enough to be seen with the naked eye. Based upon parallax measurements taken during the Hipparcos mission, it is approximately 235 light-years from the Sun.[1]
Zeta Ceti is the primary or 'A' component of a double star system designated WDS J01515-1020 (the secondary or 'B' component is HD 11366).[10] Zeta Ceti's two components are therefore designated WDS J01515-1020 Aa and Ab. Aa is officially named Baten Kaitos/ˈbeɪtənˈkeɪtɒs/, the traditional name of the entire system.[11][12]
^ abcdefCite error: The named reference vanLeeuwen2007 was invoked but never defined (see the help page).
^ abcdCite error: The named reference Jennens1975 was invoked but never defined (see the help page).
^Cite error: The named reference lu1991 was invoked but never defined (see the help page).
^Cite error: The named reference cgcvs2007 was invoked but never defined (see the help page).
^ abCite error: The named reference Massarotti2008 was invoked but never defined (see the help page).
^Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
^Cite error: The named reference Pourbaix2004 was invoked but never defined (see the help page).
^ abCite error: The named reference Luck2015 was invoked but never defined (see the help page).
^Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
^"Washington Double Star Catalog". United States Naval Observatory. Retrieved 23 February 2018.
^Kunitzsch, Paul; Smart, Tim (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, Massachusetts: Sky Pub. ISBN 978-1-931559-44-7.
^Cite error: The named reference IAU-LSN was invoked but never defined (see the help page).
ZetaCeti (ζ Ceti, abbreviated Zeta Cet, ζ Cet) is a binary star in the equatorial constellation of Cetus. It has a combined apparent visual magnitude...
Kaitos (star), the official name of ZetaCeti's primary component, and the traditional name of the entire ZetaCeti system Baten Kaitos: Eternal Wings...
violent storms. Lambda, Mu, Xi, Nu, Gamma, and Alpha Ceti represented its head; Omicron, Zeta, and Chi Ceti represented its body; Eta Eri, Tau Cet, and Upsilon...
historian Raymond Baten (born 1989), Aruban footballer Baten Kaitos, or ZetaCeti Baten Kaitos: Eternal Wings and the Lost Ocean, role-playing video game...
the Herschel 400 Catalogue. It lies about five degrees northeast from ZetaCeti. It can be seen with a small telescope at moderate magnification, with...
both magnitude and position. Such stars include Omicron Andromedae, Omicron Ceti, and Omicron Persei. In Claudius Ptolemy's (c. 100–170) Almagest, tables...
51 Delta Centauri Star 2.53 Alpha Ceti Star 2.53 Delta Leonis Star 2.55 Zeta Centauri Binary star system 2.56 Zeta Ophiuchi Star Maximum brightness 2...
C.; Holland, W. S.; Dent, W. R. F. (2004). "The debris disc around tau Ceti: a massive analogue to the Kuiper Belt". Monthly Notices of the Royal Astronomical...
stars duplicate names by mistake: Xi Arietis (duplicated as Psi Ceti) and Kappa Ceti (Kappa1 and Kappa2) (duplicated as g Tauri). He corrected these in...
Cygni — suddenly brightened in the 17th century WNC4 — Messier Object 40 Zeta Boötis — speckle binary test system Lists of astronomical objects Astronomical...
period of 3.45 days TY Coronae Borealis is a pulsating white dwarf (of ZZ Ceti) type, which is around 70% as massive as the Sun, yet has only 1.1% of its...
taking control of the Enterprise, Captain Kirk exiles them to the planet Ceti Alpha V. ("Space Seed (TOS)) 2267 Kirk discovers that Zefram Cochrane was...
planets. XLII. A system of Earth-mass planets around the nearby M dwarf YZ Ceti". Astronomy & Astrophysics. 605: L11. arXiv:1708.03336. Bibcode:2017A&A....
decreases towards the edge of the stellar disk. Red dwarf flare stars such as UV Ceti may possess prominent starspot features. The apparent brightness of a star...