31 Boötis

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Template:Short description

31 Boötis
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 4.86[2]
Characteristics
Spectral type G7 IIIa[3]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: –9.589[1] mas/yr
Dec.: +3.906[1] mas/yr
Parallax (π)6.8757±0.2796 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−1.22[2]
Details
Mass3.27[4] 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)2.60[5] cgs
TemperatureScript error: No such module "val".[1] K
Metallicity [Fe/H]−0.10[5] dex
Rotational velocity (v sin i)6.5[6] km/s
Age370[4] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

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31 Boötis is a single[8] star in the northern constellation of Boötes,[7] located 470 light years from the Sun.[1] It is visible to the naked eye as a faint, yellow-hued star with an apparent visual magnitude of 4.86.[2] The object is moving closer to the Earth with a heliocentric radial velocity of −16.5 km/s.[2] It was known to be part of a constellation between Virgo and Boötes named Mons Maenalus, it was also the brightest star in the constellation.

This is an evolved giant star with a stellar classification of G7 IIIa.[3] It is a suspected variable star of unknown type,[9] and is an X-ray source.[10] The star is 370[4] million years old with 3.27[4] times the mass of the Sun. Having exhausted the hydrogen at its core, the star has expanded to 23[1] times the Sun's radius. It is radiating 275[1] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,874 K.[1]

References

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External links

Template:Stars of Boötes