89 Virginis

Single, evolved giant star in the constellation Virgo From Wikipedia, the free encyclopedia

89 Virginis is a single[9] star in the zodiac constellation of Virgo, located 234 light years from the Sun. It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 4.959.[2] The star is moving closer to the Earth with a heliocentric radial velocity of −39 km/s.[1]

Right ascension13h 49m 52.28340s[1]
Declination−18° 08 03.0103[1]
Quick facts Constellation, Right ascension ...
89 Virginis
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 13h 49m 52.28340s[1]
Declination −18° 08 03.0103[1]
Apparent magnitude (V) 4.959[2]
Characteristics
Spectral type K0III[3]
U−B color index +0.86[4]
B−V color index +1.06[4]
Astrometry
Radial velocity (Rv)−39.45±0.17[1] km/s
Proper motion (μ) RA: −101.100[1] mas/yr
Dec.: −38.200[1] mas/yr
Parallax (π)13.9184±0.2053 mas[1]
Distance234 ± 3 ly
(72 ± 1 pc)
Absolute magnitude (MV)0.618[5]
Details
Mass1.70[6] M
Radius12[7] R
Luminosity69[6] L
Surface gravity (log g)2.6[7] cgs
Temperature4,706±13[6] K
Metallicity [Fe/H]−0.03[7] dex
Age3.40[6] Gyr
Other designations
89 Vir, BD−17°3937, GJ 9460, HD 120452, HIP 67494, HR 5196, SAO 158186[8]
Database references
SIMBADdata
Close

This is an evolved giant star with a stellar classification of K0 III,[3] having exhausted the hydrogen at its core and expanded away from the main sequence. It is a red clump star, which indicates it is generating energy through helium fusion at its core.[5] This object is 3.4 billion years old with 1.7[6] times the mass of the Sun and 12[7] times the Sun's radius. It is radiating 69 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4706 K.[6]

References

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