HD 149143

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Template:Short description

HD 149143 / Rosalíadecastro
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 7.89[3]
Characteristics
Spectral type G0 IV[3] or G3V[4]
B−V Template:Engvar 0.680[3]
Astrometry
Radial velocity (Rv)12.104±0.0054[5] km/s
Proper motion (μ) RA: −9.240 mas/yr[6]
Dec.: −86.678 mas/yr[6]
Parallax (π)13.6279±0.0247 mas[6]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)3.87[3]
Details
Mass1.1±0.1[3] Template:Solar mass
Radius1.302Script error: No such module "Su".[7] Template:Solar radius
Luminosity2.278±0.008[7] Template:Solar luminosity
Surface gravity (log g)4.10[3] cgs
Temperature6,213[7] K
Metallicity [Fe/H]0.20±0.05[3] dex
Rotational velocity (v sin i)3.9[3] km/s
Age7.6±1.2[3] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata
Exoplanet Archivedata

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HD 149143, also called Rosalíadecastro, is a star with a close orbiting exoplanet in the Ophiuchus constellation. Its apparent visual magnitude is 7.89[3] (a binocular object) and the absolute magnitude is 3.87.[9] The system is located at a distance of 239 light years from the Sun based on parallax measurements, and it is drifting further away with a radial velocity of 12 km/s.[5]

On December 17, 2019, as part of the IAU's NameExoWorlds project, the star HD 149143 was given the name Rosalíadecastro in honour of the Galician poet Rosalía de Castro, who was a significant figure of Galician culture and prominent writer in Galician overall, but in Spanish too, whose work often referenced the night and celestial objects. The exoplanet companion was named Riosar in honour of the Sar River in Galicia that was present in much of the literary work of the author Rosalía de Castro.[10][11]

This is a slightly evolved star with a stellar classification of G0 that is overluminous for a high-metallicity G-type dwarf.[9] It has 1.1[3] times the mass of the Sun and 1.3[7] times the Sun's radius. The star has an estimated age of around 7.6 billion years and is spinning with a projected rotational velocity of 3.9 km/s.[3] It is radiating 2.3 times the luminosity of the Sun from its photosphere at an effective temperature of 6,213 K.[7]

Planetary system

HD 149143 b, the planet that orbits HD 149143, was discovered by the N2K Consortium during their search for short-period gas giant planets around metal-rich stars.[3] The planet was independently discovered by the Elodie metallicity-biased search for transiting Hot Jupiters.[9]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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See also

Template:Sister project

References

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Template:Sky Template:Stars of Ophiuchus