Theta Ophiuchi

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Template:Short description

Theta Ophiuchi
Template:Location mark
Location of θ Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.25 - 3.31[2]
Characteristics
Spectral type B2 IV[3]
U−B Template:Engvar −0.86[4]
B−V Template:Engvar −0.23[4]
Variable type β Cep[2]
Astrometry
Radial velocity (Rv)−2[5] km/s
Proper motion (μ) RA: −7.37[1] mas/yr
Dec.: −23.94[1] mas/yr
Parallax (π)7.48±0.17 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−2.4[6]
Details
θ Oph Aa
MassScript error: No such module "val".[7] Template:Solar mass
RadiusScript error: No such module "val".[7] Template:Solar radius
LuminosityScript error: No such module "val".[7] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[8] cgs
TemperatureScript error: No such module "val".[8] K
Metallicity [Fe/H]Script error: No such module "val".[9] dex
Rotational velocity (v sin i)30[10] km/s
AgeScript error: No such module "val".[7] Myr
θ Oph B
Mass5.4[7] Template:Solar mass
RadiusScript error: No such module "val".[7] Template:Solar radius
LuminosityScript error: No such module "val".[7] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[7] cgs
Temperature17,700[7] K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Rotational velocity (v sin i)150[7] km/s
AgeScript error: No such module "val".[7] Myr
Other designations
Template:Odlist[11]
Database references
SIMBADdata

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Theta Ophiuchi, Latinized from θ Ophiuchi, is a multiple star system in the equatorial constellation of Ophiuchus. It lies on the "right foot" of the serpent-bearer, just southwest of Kepler's Star, the nova of 1604. This star has an apparent visual magnitude of +3.3,[6] making it readily visible to the naked eye. Based upon parallax measurements from the Hipparcos mission, it is roughly Script error: No such module "convert". from Earth.[1] It is 1.8 degrees south of the ecliptic and therefore subject to lunar occultations and (very rarely) occulted by a planet. The next occultation by a planet will be by Mars on 3 October 2078.[12]

Theta Ophiuchi appears to be a triple star system. The brightest component is a spectroscopic binary with an orbital period of 56.71 days and an eccentricity of 0.17. The third component is 5.5 magnitude star with a stellar classification of B5. Its angular separation from the binary pair is 0.15 arcseconds.[13] This system is a proper motion member of the Upper Scorpius sub-group in the Scorpius–Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.[6]

File:ThetaOphLightCurve.png
A light curve for Theta Ophiuchi, plotted from Hipparcos data[14]

The primary component of this system is a variable star of the Beta Cephei type with a period of just 3h 22m.[15] It has an estimated 8.0 to 8.6 times the mass of the Sun and 4.98 to 5.23 times the Sun's radius. Although only 15.8 to 24 million years old,[7] it has begun to evolve away from the main sequence and has become a subgiant star with a stellar classification of B2 IV.[3] This massive star is radiating between 4,740 and 6,230 times the luminosity of the Sun from its photosphere[7] at an effective temperature of about 22,260 K,[8] giving it the blue-white hue of a B-type star.[16]

According to Richard H. Allen's Star Names: Their Lore and Meaning (1899), θ Oph together with ξ Oph formed the Sogdian Wajrik "the Magician", the Khorasmian Markhashik "the Serpent-bitten" and with η Oph the Coptic Tshiō, "the Snake", and Aggia, "the Magician".[17] With ζ Oph, η Oph, and ξ Oph it formed the Persian Garafsa, the Serpent-tamer;[17] a 1971 NASA list of star names includes the name Garafsa for θ Oph.[18]

References

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Template:Stars of Ophiuchus