HD 89307

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Template:Short description

HD 89307
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Leo
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 7.02[2]
Characteristics
Spectral type G0V[3]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[1] km/s
Proper motion (μ) RA: −272.659 mas/yr[1]
Dec.: −39.333 mas/yr[1]
Parallax (π)31.4134±0.0226 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)4.57[4]
Details[4]
MassScript error: No such module "val". Template:Solar mass
RadiusScript error: No such module "val".[5] Template:Solar radius
LuminosityScript error: No such module "val".[5] 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".[2] dex
RotationScript error: No such module "val".
Rotational velocity (v sin i)Script error: No such module "val". km/s
AgeScript error: No such module "val".[2]
6.76[4] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[6]
Database references
SIMBADdata

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HD 89307 is a star in the equatorial constellation of Leo. It is too faint to be viewed with the naked eye except under ideal conditions, having an apparent visual magnitude of 7.02.[2] The star is located at a distance of Script error: No such module "convert". from the Sun based on parallax, and is drifting further away with a radial velocity of +23 km/s.[1]

This is an ordinary G-type main-sequence star with a stellar classification of G0V.[3] It is chromospherically inactive and appears older than the Sun with a rotation period of 23.7 days.[4] The star has about the same mass[4] as the Sun and is 8% larger. It is radiating 1.35[5] times the Sun's luminosity from its photosphere at an effective temperature of 5,950 K.[4]

Planetary system

In December 2004, using the radial velocity method, it was found to have a long-period giant planet in orbit around it.[4] The parameters of HD 89307 b were updated in 2012,[7] and in 2023 its inclination and true mass were determined via astrometry.[8]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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See also

References

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  1. a b c d e f Template:Cite Gaia DR3
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  5. a b c Template:Cite Gaia DR2
  6. Template:Cite simbad
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External links

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Template:Sky Template:Stars of Leo