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31 Boötis

Star in the constellation Boötes From Wikipedia, the free encyclopedia

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.

Right ascension14h 41m 38.75049s[1]
Declination+08° 09 42.3409[1]
Quick facts Constellation, Right ascension ...
31 Boötis
Location of 31 Boötis (circled in red)
Observation data
Epoch J2000      Equinox ICRS
Constellation Boötes
Right ascension 14h 41m 38.75049s[1]
Declination +08° 09 42.3409[1]
Apparent magnitude (V) 4.86[2]
Characteristics
Spectral type G7 IIIa[3]
B−V color index 0.992±0.038[2]
Astrometry
Radial velocity (Rv)−16.5±1.8[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]
Distance470 ± 20 ly
(145 ± 6 pc)
Absolute magnitude (MV)−1.22[2]
Details
Mass3.27[4] M
Radius23.25+0.40
−0.49
[1] R
Luminosity274.9±12.6[1] L
Surface gravity (log g)2.60[5] cgs
Temperature4,874+53
−41
[1] K
Metallicity [Fe/H]−0.10[5] dex
Rotational velocity (v sin i)6.5[6] km/s
Age370[4] Myr
Other designations
31 Boo, NSV 6769, BD+08°2903, FK5 3163, GC 19789, HD 129312, HIP 71832, HR 5480, SAO 120601[7]
Database references
SIMBADdata
Close

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]

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