HD 102117

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Template:Short description

HD 102117 / Uklun
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 7.47[1]
Characteristics
Evolutionary stage subgiant[2]
Spectral type G6V[3]
B−V Template:Engvar Script error: No such module "val".[1]
Variable type Constant[4]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: −63.574 mas/yr[2]
Dec.: −70.331 mas/yr[2]
Parallax (π)25.3531±0.0178 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)4.48[1]
Details
MassScript error: No such module "val".[5]
Script error: No such module "val".[6] Template:Solar mass
Radius1.27[7] Template:Solar radius
Luminosity1.54[7] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[7] cgs
TemperatureScript error: No such module "val".[5] K
Metallicity [Fe/H]Script error: No such module "val".[6] dex
Rotational velocity (v sin i)Script error: No such module "val".[7] km/s
AgeScript error: No such module "val".[5] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata
Exoplanet Archivedata

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HD 102117 or Uklun Template:IPAc-en is a star in the southern constellation of Centaurus. With an apparent visual magnitude of 7.47,[1] it is too dim to be seen without binoculars or a small telescope. It is located at a distance of approximately 129 light-years from the Sun based on parallax. HD 102117 is drifting further away with a radial velocity of +50 km/s,[2] having come to within Script error: No such module "convert". some 692,000 years ago.[1] It has one known planet.[6]

The stellar classification of HD 102117 is G6V,[9] which matches the spectrum of an ordinary G-type main-sequence star. It is roughly five[5] billion years old and is spinning with a projected rotational velocity of 0.9 km/s.[7] The star shows only a low level of chromospheric activity[6] and is photometrically stable,[4] meaning it doesn't vary significantly in brightness. It appears metal-enriched,[4] showing a higher abundance of heavy elements compared to the Sun.

Planetary system

In 2004, the Anglo-Australian Planet Search announced a planet orbiting the star.[4] A short time later the HARPS team also announced the presence of a planet around this star. Both groups detected this planet with the radial velocity method.[6]

HD 102117, and its planet HD 102117b, were chosen as part of the 2019 NameExoWorlds campaign organised by the International Astronomical Union, which assigned each country a star and planet to be named. HD 102117 was assigned to Pitcairn Islands. The winning proposal named the star Uklun, from the word aklan 'we/us' in the Pitcairn language, and the planet Leklsullun Template:IPAc-en, from the phrase lekl salan 'child/children' (lit. 'little person').[10]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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See also

References

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External links

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Template:Sky Template:Stars of Centaurus