Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Monoceros |
Right ascension | 07h 10m 13.68177s[1] |
Declination | −04° 14′ 13.5829″[1] |
Apparent magnitude (V) | 4.92[2] |
Characteristics | |
Evolutionary stage | horizontal branch[3] |
Spectral type | K0III[4] |
U−B color index | +0.78[2] |
B−V color index | +1.03[2] |
Astrometry | |
Radial velocity (Rv) | +77.74[5] km/s |
Proper motion (μ) | RA: −0.714[1] mas/yr Dec.: +217.298[1] mas/yr |
Parallax (π) | 16.8419 ± 0.1692 mas[1] |
Distance | 194 ± 2 ly (59.4 ± 0.6 pc) |
Absolute magnitude (MV) | 0.94[6] |
Details[7] | |
Mass | 1.07±0.20 M☉ |
Radius | 10.25±0.11[1] R☉ |
Luminosity | 46.36±0.56[1] L☉ |
Surface gravity (log g) | 2.53±0.10 cgs |
Temperature | 4,714±46 K |
Metallicity [Fe/H] | −0.25±0.03 dex |
Rotational velocity (v sin i) | 2.33±0.50 km/s |
Age | 5.75±2.85 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
20 Monocerotis is a single[9] star located about 194[1] light years away from the Sun in the equatorial constellation of Monoceros. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.92.[2] The star is receding from the Earth with a heliocentric radial velocity of +78 km/s.[5]
This object is an aging giant star with a stellar classification of K0 III.[4] It is a red clump giant,[3] which indicates it is on the horizontal branch and is generating energy through helium fusion at its core. The star is around six[7] billion years old with 1.1 times the mass of the Sun. After exhausting the supply of hydrogen at its core, it has expanded to 10.3[1] times the Sun's radius. It is radiating 46[1] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,714 K.[7]
In addition to the primary, three visual companions have been reported: component B, with magnitude 12.93 and separation 67.8", C, with magnitude 10.16 and separation 167.9", and D, with magnitude 12.46 and separation 102.3".[10]