HD 154857

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Template:Short description

HD 154857
Observation data
Epoch J2000      Equinox J2000
Constellation Ara[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 7.25[1]
Characteristics
Evolutionary stage subgiant[2]
Spectral type G5IV-V[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: +87.442[2] mas/yr
Dec.: −55.861[2] mas/yr
Parallax (π)15.8176±0.0197 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)3.07[3]
Details
MassScript error: No such module "val".[5] Template:Solar mass
RadiusScript error: No such module "val".[4] Template:Solar radius
LuminosityScript error: No such module "val".[4] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[4] cgs
TemperatureScript error: No such module "val".[4] 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".[4] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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HD 154857 is a star with two exoplanetary companions in the southern constellation of Ara. It is too dim to be visible with the naked eye having an apparent visual magnitude of 7.25.[1] The star is located at a distance of 206 light years from the Sun based on parallax measurements, and is drifting further away with a radial velocity of +28 km/s.[2]

This is a G-type star with a stellar classification of G5IV-V.[3] The absolute magnitude of this star is two magnitudes above the main sequence, which suggests that the star is evolving toward the subgiant stage.[3] It is a metal-poor thin disk star[9] approximately six billion years old and is chromopherically quiet although not in a Maunder Minimum state.[4] The star is larger, more massive, and more luminous than the Sun. It is spinning with a projected rotational velocity of 1.4 km/s.[7]

Planetary system

The discovery of one confirmed and one unconfirmed Jovian exoplanet was reported in 2004[3] and 2007[10] respectively. The former planet HD 154857 b has mass >1.8 times that of Jupiter. It orbits the star 20% further than Earth-Sun distance, taking 409 days with 47% eccentricity. The additional object (HD 154857 c) was confirmed as a planetary companion in January 2014.[5]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet Template:OrbitboxPlanet

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See also

References

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External links

Template:Sky Template:Stars of Ara