HD 170469

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Template:Short description

HD 170469
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 8.21[2]
Characteristics
Spectral type G5V + K5V[3]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[3] km/s
Proper motion (μ) RA: Script error: No such module "val".[1] mas/yr
Dec.: Script error: No such module "val".[1] mas/yr
Parallax (π)16.5886±0.0408 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)4.23[2]
Orbit[4]
PrimaryHD 170469
CompanionHD 170469 B
Period (P)114000 yr
Semi-major axis (a)43.1″
Details
A
Mass1.10[5] Template:Solar mass
Radius1.24[5] Template:Solar radius
LuminosityScript error: No such module "val".[1] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[5] cgs
TemperatureScript error: No such module "val".[3] K
Metallicity [Fe/H]Script error: No such module "val".[3] dex
AgeScript error: No such module "val".[2] or Script error: No such module "val".[6] Gyr
B
Mass0.42[7] Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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HD 170469 is a probable binary star[7][4] system in the equatorial constellation of Ophiuchus. It is too faint to be viewed with the naked eye, having an apparent visual magnitude of 8.21.[2] The system is located at a distance of 197 light years away from the Sun based on parallax. It is drifting closer with a radial velocity of −59 km/s,[3] and is expected to come to within Script error: No such module "convert". in about 959,000 years.

The primary, component A, is a G-type main-sequence star with a stellar classification of G5V,[3] indicating it is generating energy through core hydrogen fusion. Estimates of the star's age range from five[2] to almost nine[6] billion years. It has 1.10 times the mass of the Sun and 1.24 times the Sun's radius.[5] The star has a higher than solar metallicity.[3] It is radiating 1.64[1] times the Sun's luminosity from its photosphere at an effective temperature of 5,786 K.[3]

The secondary companion, component B, is located at an angular separation of Script error: No such module "val". along a position angle of Script error: No such module "val". from the primary, as of 2018.[3] Initially it was thought to be a red dwarf of spectral class M1,[4] but was later determined to be a K-type main-sequence star with a class of K5V.[3] This star lies at a projected separation of Script error: No such module "val".[4] from the primary, and is orbiting with an estimated period of around 114,000 years.[7]

Planetary system

In 2007, a planet was discovered by the N2K Consortium, led by principal investigators Debra Fischer and Gregory P. Laughlin.[9] It was spotted using the radial velocity method, and was independently confirmed in 2014.[4]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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See also

References

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Template:Ophiuchus Template:Sky