HD 231701

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Template:Short description

HD 231701 / Uruk
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagitta[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 8.97[1]
Characteristics
Evolutionary stage main sequence[3][2]
Spectral type F8 V[1]
B−V Template:Engvar Script error: No such module "val".[1]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: Script error: No such module "val". mas/yr[2]
Dec.: Script error: No such module "val". mas/yr[2]
Parallax (π)9.2189±0.0160 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)3.64[1]
Details
MassScript error: No such module "val".[4] Template:Solar mass
RadiusScript error: No such module "val".[5] Template:Solar radius
LuminosityScript error: No such module "val".[5] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[6] cgs
TemperatureScript error: No such module "val".[5] K
Metallicity [Fe/H]Script error: No such module "val".[7] dex
Rotational velocity (v sin i)4.26[6] km/s
AgeScript error: No such module "val".[4] or 4.5[3] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata
Exoplanet Archivedata

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HD 231701 is a yellow-white hued star in the northern constellation of Sagitta, near the southern constellation border with Aquila. With an apparent visual magnitude of 8.97,[1] it is too dim to be viewed with the naked eye, but can be seen with powerful binoculars or a small telescope. Parallax measurements provide a distance estimate of approximately 354 light-years from the Sun, but it is drifting closer with a radial velocity of −63 km/s.[2] It is predicted to come as close as Script error: No such module "convert". in 1.345 million years.[1]

HD 231701 is named Uruk. The name was selected in the NameExoWorlds campaign by Iraq, during the 100th anniversary of the IAU. Uruk was an ancient city of the Sumer and Babylonian civilizations in Mesopotamia.[9][10]

This object is an ordinary F-type main-sequence star with a stellar classification of F8 V.[1] It is around three[4] to 4.5 billion years old and may be evolving onto the subgiant branch.[3] It is spinning with a projected rotational velocity of 4 km/s[6] and has low chromospheric activity.[3] HD 231701 has 1.2[4] times the mass of the Sun and 1.45[5] times the Sun's radius. It is radiating 2.6 times the luminosity of the Sun from its photosphere at an effective temperature of 6,081 K.[5]

In 2007, the N2K Consortium used the radial velocity technique to discover a Jupiter-like planet orbiting at a distance of Script error: No such module "val". from the star with a period of 141.6 days.[3]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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See also

References

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  5. a b c d e Template:Cite Gaia DR2
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External links

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Template:Sky

Template:Stars of Sagitta