13 Ceti
Observation data Epoch J2000.0 Equinox J2000.0 | ||
---|---|---|
Constellation | Cetus | |
Right ascension | 00h 35m 14.87968s[1] | |
Declination | −03° 35′ 34.2367″[1] | |
Apparent magnitude (V) | 5.20[2] (5.61 + 6.90)[3] | |
Characteristics | ||
Evolutionary stage | Main sequence | |
Spectral type | F6 V + G4 V + K3.5 V[4][5] | |
B−V color index | 0.567±0.008[2] | |
Variable type | RS CVn[6] | |
Absolute magnitude (MV) | 3.56[2] | |
Argument of periastron (ω)(secondary) | 283.8°° | |
Semi-amplitude (K1)(primary) | 43.98±0.39 km/s | |
Details | ||
Aa | ||
Gyr | ||
Database references | ||
SIMBAD | data |
13 Ceti is a
light years from the Sun based on stellar parallax, and is drifting further away with a radial velocity of +10.4 km/s.[7] It shares a common motion with the Hyades moving group,[5] although it is too old to be a member.[11]
This star was identified as a visual binary system by
variable star designation of BU Cet.[6] The star was detected as a source of soft X-ray emission by EXOSAT.[13] It has 18%[5] more mass than the Sun and is estimated to be about four[2]
billion years old.
In 1907,
spectroscopic binary, making this a triple star system. This is a double-lined spectroscopic binary with a period of 2.1 days and a circularized orbit. The companion signature was confirmed using the separated fringe packet technique with the CHARA array.[14] It is most likely a K-type main-sequence star with a class of K3.5 V and 70% of the mass of the Sun.[5]
The secondary member of the visual binary, designated component B, is a
″ from the primary along a position angle of 322°.[3]
References
- ^ S2CID 18759600.
- ^ S2CID 119257644.
- ^ doi:10.1086/323920, retrieved 2015-07-22.
- ^ Bibcode:1993A&AS..100..173S.
- ^ , A96.
- ^ doi:10.1086/191866.
- ^ S2CID 15290475.
- ^ .
- Bibcode:1991A&A...248..485D.
- ^ "13 Cet". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-11-05.
- Bibcode:2001ASPC..223.1477M.
- doi:10.1086/144671.
- S2CID 121806441.
- S2CID 15622813, 24.
- doi:10.1086/143133.