HD 101930

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Template:Short description

HD 101930
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 8.21[2]
Characteristics
Spectral type K2 V+[3]
B−V Template:Engvar +0.91[4]
Astrometry
Radial velocity (Rv)+18.36[5] km/s
Proper motion (μ) RA: +16.680 mas/yr[1]
Dec.: +349.125 mas/yr[1]
Parallax (π)33.3814±0.0180 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+5.88[2]
Details
Radius0.87Script error: No such module "Su".[6] Template:Solar radius
Luminosity0.43±0.01[7] Template:Solar luminosity
Surface gravity (log g)4.40±0.11[8] cgs
Temperature5,079±62[5] K
Metallicity [Fe/H]+0.1±0.03[9] dex
Rotational velocity (v sin i)2[10] km/s
Age5.4±4.4[7] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
CD-57°4096, GJ 3683, HIP 57172, LTT 4350, NLTT 28356, SAO 239322[11]
Database references
SIMBADdata
ARICNSdata

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HD 101930, also known as GJ 3683, is an orange hued star with an orbiting exoplanet located in the southern constellation Centaurus. It has an apparent magnitude of 8.21,[2] making it faintly visible in binoculars but not to the naked eye. The system is located relatively close at a distance of 98 light years[1] but is receding with a heliocentric radial velocity of Script error: No such module "val"..[5] It has a relatively large proper motion, traversing the celestial sphere with an angular velocity of Script error: No such module "val".·yr−1.[12]

HD 101930 has a stellar classification of K2 V+,[3] indicating that it is an ordinary K-type main-sequence star. It has an estimated age of 5.4 billion years,[7] which is slightly older than the Sun. The object has 87% the radius of the Sun[6] and an effective temperature of Script error: No such module "val"..[5] When combined, these parameters yield a luminosity 43% that of the Sun from its photosphere.[7] As expected with planetary hosts, HD 101930 is metal enriched, having a metallicity 26% above solar levels.[9] The star's projected rotational velocity is similar to the Sun's, having a value of Script error: No such module "val"..[10]

A 2007 multicity survey found a co-moving companion located Script error: No such module "val". away,[13] making it a binary star. It has a class of M0-1[14] and a mass of Template:Solar mass.[13]

Planetary system

In 2005, the discovery of an exoplanet orbiting the star was announced. This is another discovery using the radial velocity method with the HARPS spectrograph. As the inclination of the orbital plane is unknown, only a lower bound on the mass can be determined. It has at least 30% of the mass of Jupiter.[5]

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