HD 187123

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Template:Short description

HD 187123
File:HD 187123 planetary system (artist's impression).jpg
HD 187123 has a planetary system with at least two planets in it. Artist's rendition of planets HD 187123 b and c.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cygnus[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 7.83[1]
Characteristics
Spectral type G2V[3]
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)21.7166±0.0157 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)4.41[1]
Details
MassScript error: No such module "val".[4] 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".[5] dex
Rotational velocity (v sin i)Script error: No such module "val".[5] km/s
AgeScript error: No such module "val".[4] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[6]
Database references
SIMBADdata

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HD 187123 is a single,[7] yellow-hued star with two exoplanetary companions in the northern constellation of Cygnus. It has an apparent visual magnitude of 7.83,[1] making it an 8th magnitude star that is too faint to be visible with the naked eye. However, it should be easy target with binoculars or small telescope. The system is located at a distance of 150 light years from the Sun based on parallax measurements, but is drifting closer with a radial velocity of −17 km/s.[2]

Description

This is an ordinary G-type main-sequence star with a stellar classification of G2V.[3] The physical properties of this star are sufficiently similar to the Sun that it has been considered a solar analog, although the metallicity is higher.[8] It is estimated to be five or six billion years old and is spinning with a projected rotational velocity of 2 km/s.[5] The star has a similar mass to the Sun but is slightly larger with 117% of the Sun's radius. It is radiating 1.44 times the luminosity of the Sun from its photosphere at an effective temperature of 5,853 K.[4]

Planetary system

In 1998 the California and Carnegie Planet Search team, after following a suggestion by Kevin Apps, a Briton who at the time was an undergraduate student[9] found a possible planet orbiting the star.[10] There were also indications of another, more distant body orbiting the star and this claim was published in 2006.[11] This planet was confirmed in 2009.[12] The presence of water has been detected in the atmosphere of HD 187123 b with high confidence.[13]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet Template:OrbitboxPlanet

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See also

References

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  5. a b c Script error: No such module "Citation/CS1".
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External links

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Template:Sky Template:Stars of Cygnus