Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Virgo |
Right ascension | 15h 02m 54.03756s[1] |
Declination | +02° 05′ 28.6957″[1] |
Apparent magnitude (V) | 4.40[2] |
Characteristics | |
Spectral type | K0.5 IIIb Fe–0.5[3] |
B−V color index | 1.04[2] |
Astrometry | |
Radial velocity (Rv) | −16.2±0.3[1] km/s |
Proper motion (μ) | RA: −55.569 mas/yr[1] Dec.: +13.628 mas/yr[1] |
Parallax (π) | 16.7474 ± 0.129 mas[1] |
Distance | 195 ± 2 ly (59.7 ± 0.5 pc) |
Details | |
Mass | 1.67[2] M☉ |
Radius | 13.78±0.14[4] R☉ |
Luminosity | 80.4±1.8[4] L☉ |
Surface gravity (log g) | 2.7[5] cgs |
Temperature | 4,655±24[4] K |
Metallicity [Fe/H] | −0.3[5] dex |
Age | 4.52[2] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
110 Virginis is a star in the zodiac constellation Virgo, located 195[1] light-years away from Earth. It is visible to the naked eye as an orange-hued star with an apparent visual magnitude of 4.40.[2] The star is moving closer to the Earth with a heliocentric radial velocity of −16 km/s.[1]
The stellar classification of 110 Virginis is K0.5 IIIb Fe–0.5,[3] indicating that this is an evolved giant star with a mild underabundance of iron in its spectrum. At the age of 4.5[2] billion years old, it belongs to a sub-category of giants called the red clump, which means it is on the horizontal branch and is generating energy through the helium fusion at its core.[7] Compared to the Sun, it has 167%[2] of the mass but has expanded to 14 times the size. The enlarged photosphere has an effective temperature of 4,655 K and is radiating 80 times the Sun's luminosity.[4]
DR3
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