HD 17092

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Template:Short description

HD 17092
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Perseus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 7.73[2]
Characteristics
Evolutionary stage Giant[2]
Spectral type K0III[3]
B−V Template:Engvar Script error: No such module "val".[4]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] 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)4.3499±0.0516 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+1.76[4]
Details[6]
MassScript error: No such module "val". Template:Solar mass
RadiusScript error: No such module "val".[1] Template:Solar radius
LuminosityScript error: No such module "val".[1] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val". cgs
TemperatureScript error: No such module "val". K
Metallicity [Fe/H]Script error: No such module "val". dex
Rotation505 days[4]
Rotational velocity (v sin i)Script error: No such module "val". km/s
AgeScript error: No such module "val". Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist
Database references
SIMBADdata

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HD 17092 is a star in the constellation of Perseus. It has an orange hue but is visible only with binoculars or better equipment, having an apparent visual magnitude of 7.73.[2] The distance to this star is approximately 750 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +5.5 km/s.[5]

This object is an aging giant star with a stellar classification of K0III,[3] which means it has exhausted the supply of hydrogen at its core then cooled and expanded off the main sequence.[4] It is roughly six billion years old with 1.2[6] times the mass of the Sun and has expanded to 12 times the Sun's radius.[1] The star is radiating 57[1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,630 K.[6]

Planetary system

On 6 May 2007, a planet HD 17092 b was discovered with the Hobby-Eberly Telescope by Niedzielski who used the wobble method. This planet is a massive gas giant and orbits at 1.29 astronomical units from the star with a period of about 360 days.[4]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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References

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  1. a b c d e f g h i Template:Cite Gaia DR2
  2. a b c Script error: No such module "citation/CS1".
  3. a b Script error: No such module "citation/CS1".
  4. a b c d e Script error: No such module "Citation/CS1".
  5. a b Script error: No such module "citation/CS1".
  6. a b c Script error: No such module "citation/CS1".

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Template:Sky Template:Stars of Perseus