Chi Tauri

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Chi Tauri
Template:Location mark
Location of χ Tauri (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
χ Tau A
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 5.378[2]
χ Tau B
Right ascension Template:RA[3]
Declination Template:DEC[3]
Apparent magnitude (V) 8.423[4]
Characteristics
χ Tau A
Spectral type B9V[4]
U−B Template:Engvar -0.12[5]
B−V Template:Engvar -0.04[5]
χ Tau B
Spectral type F8 + G6 + K4 + K4[4]
U−B Template:Engvar +0.10[5]
B−V Template:Engvar +0.63[5]
Astrometry
χ Tau A
Radial velocity (Rv)Script error: No such module "val".[4] km/s
Proper motion (μ) RA: +20.953[1] mas/yr
Dec.: −16.495[1] mas/yr
Parallax (π)11.0472±0.1599 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)Script error: No such module "val".[4]
χ Tau B
Radial velocity (Rv)Script error: No such module "val".[4] km/s
Proper motion (μ) RA: 15.766[3] mas/yr
Dec.: −20.396[3] mas/yr
Parallax (π)11.5348±0.0857 mas[3]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)Combined: Script error: No such module "val".
Ba: Script error: No such module "val".
Bb: Script error: No such module "val".
Bc: 7.87 / 7.87[4]
Orbit[4]
Primaryχ Tau Ba
Companionχ Tau Bb
Period (P)17.602309 ± 0.000036 d
Eccentricity (e)Script error: No such module "val".
Inclination (i)Script error: No such module "val".°
Periastron epoch (T)Script error: No such module "val".
Argument of periastron (ω)
(secondary)
Script error: No such module "val".°
Semi-amplitude (K1)
(primary)
Script error: No such module "val". km/s
Semi-amplitude (K2)
(secondary)
Script error: No such module "val". km/s
Orbit[4]
Primaryχ Tau Bab
Companionχ Tau Bc
Period (P)Script error: No such module "val".
Eccentricity (e)Script error: No such module "val".
Inclination (i)Script error: No such module "val".°
Periastron epoch (T)Script error: No such module "val".
Argument of periastron (ω)
(secondary)
Script error: No such module "val".°
Semi-amplitude (K1)
(primary)
Script error: No such module "val". km/s
Details
AgeScript error: No such module "val".[4] Myr
χ Tau A
MassScript error: No such module "val".[4] Template:Solar mass
Radius2.15[6] Template:Solar radius
Surface gravity (log g)4.15 ± 0.14[7] cgs
TemperatureScript error: No such module "val".[4] K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Rotational velocity (v sin i)263[7] km/s
χ Tau Ba
Mass1.19[4] Template:Solar mass
Surface gravity (log g)4.5[4] cgs
TemperatureScript error: No such module "val".[4] K
Rotational velocity (v sin i)Script error: No such module "val".[4] km/s
χ Tau Bb
Mass1.02[4] Template:Solar mass
Surface gravity (log g)4.5[4] cgs
TemperatureScript error: No such module "val".[4] K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Rotational velocity (v sin i)Script error: No such module "val".[4] km/s
χ Tau Bc
Mass~0.70 / 0.70[4] Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist
Database references
SIMBADχ Tau A
χ Tau B

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Chi Tauri, Latinised from χ Tauri, is a star system in the constellation of Taurus. Parallax measurements made by the Hipparcos spacecraft put it at a distance of about Script error: No such module "convert". from Earth. The primary component has an apparent magnitude of about 5.4,[2] meaning it is visible with the naked eye.

The main component of the system is Chi Tauri A. It is a B-type main-sequence star. Its mass is 2.6 times that of the Sun and its surface glows with an effective temperature of Script error: No such module "val".. It may be a binary star itself, as suggested from astrometric data from Hipparcos, although no orbit could be derived.[4]

The secondary component of the system is Chi Tauri B, separated about 19″[4] from Chi Tauri A. It was thought to be a post-T Tauri star from its unusual spectrum,[8] but later studies ruled this out.[4] It is a double-lined spectroscopic binary—the two stars are not resolved but their spectra have periodic Doppler shifts indicating orbital motion. The two stars are an F-type star and a G-type star, respectively, and are designated Ba and Bb.[4]

The radial velocity of Chi Tauri B has a slow drift indicating the presence of another star in the system. Designated Chi Tauri Bc, this massive object is too dim to be detected, but it appears in Chi Tauri B's spectrum as an infrared excess. Because of this infrared excess, this unseen component is thought to be a pair of K-type main-sequence stars both with masses 70% of the Sun's. The stars within the system appear to be dynamically interacting.[4]

Naming

  • With φ, κ1, κ2 and υ, it composed the Arabic were the Arabs' Al Kalbain, the Two Dogs.[9] According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Kalbain were the title for five stars: φ as Alkalbain I, this star (χ) as Alkalbain II, κ1 as Alkalbain III, κ2 as Alkalbain IV and υ as Alkalbain V.[10]Script error: No such module "Unsubst".
  • In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Whetstone, refers to an asterism consisting of χ Tauri, ψ Tauri, 44 Tauri and φ Tauri. Consequently, the Chinese name for χ Tauri itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx).[11]

References

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Template:Stars of Taurus