HD 29587

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Template:Short description

HD 29587
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 7.29[1]
Characteristics
Evolutionary stage main sequence[2]
Spectral type G2 V[3]
B−V Template:Engvar 0.633[3]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: +534.631[2] mas/yr
Dec.: −414.946[2] mas/yr
Parallax (π)36.6470±0.0410 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)5.08[3]
Orbit[4]
Period (P)Script error: No such module "val".
Eccentricity (e)0.713±0.006[5]
Periastron epoch (T)JD Script error: No such module "val".
Argument of periastron (ω)
(secondary)
Script error: No such module "val".°
Semi-amplitude (K1)
(primary)
Script error: No such module "val". km/s
Details[3]
Mass1.033±0.010[5] M
Radius0.91 Template:Efn Template:Solar radius
Luminosity0.798Script error: No such module "Su". 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
AgeScript error: No such module "val". Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[6]
Database references
SIMBADdata
Exoplanet Archivedata

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HD 29587 is a Sun-like[7] star with a candidate brown dwarf companion[8] in the northern constellation of Perseus. It has an apparent visual magnitude of 7.29,[1] which means it is too faint to be viewed with the naked eye. Based upon an annual parallax shift of Script error: No such module "val".,[2] it is located 89.8 light years away. The star is moving away from the Earth with a heliocentric radial velocity of +113 km/s,[2] having come to within Script error: No such module "convert". some 148,000 years ago.[1] It is a hyper-velocity halo[7] star moving at a rate of 170 km/s relative to the local standard of rest.[9]

This ancient star has a stellar classification of G2 V,[3] matching a G-type main-sequence star. It has 78% of the mass of the Sun and is radiating 80% of the Sun's luminosity from its photosphere at an effective temperature of 5,709 K.[3]

Planetary system

Formerly an IAU radial velocity standard, this star was found to have a variable radial velocity due to a suspected orbiting companion.[8] The a sin i value for the unseen object is Script error: No such module "convert".,[4] where a is the semimajor axis and i is the orbital inclination – providing a lower bound for the semimajor axis. The secondary object most likely has a mass in the range Script error: No such module "val"., making it a probable brown dwarf.[10]

The HD 29587 planetary system[10]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination
(°)
Radius
b ≥ 55.2±9.2[5] MJ 2.57 Template:Efn Script error: No such module "val". Script error: No such module "val".

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An artistic concept of the brown dwarf HD 29587 B

Notes

Template:Notelist

References

  1. a b c d Template:Cite XHIP
  2. a b c d e f g h i Template:Cite Gaia DR3
  3. a b c d e f Script error: No such module "Citation/CS1".
  4. a b Script error: No such module "Citation/CS1".
  5. a b c Script error: No such module "citation/CS1".
  6. Script error: No such module "citation/CS1".
  7. a b Script error: No such module "Citation/CS1".
  8. a b Script error: No such module "Citation/CS1".
  9. Script error: No such module "Citation/CS1".
  10. a b Script error: No such module "Citation/CS1".

Template:Stars of Perseus