Xi Mensae
Star in the constellation Mensa / From Wikipedia, the free encyclopedia
ξ Mensae, Latinized as Xi Mensae, is a single[7] star in the southern circumpolar constellation of Mensa. It has a yellow-orange hue and is just barely visible to the naked eye as a dim point of light with an apparent visual magnitude of 5.84.[2] This object is located about 366 light years away from the Sun based on parallax, but is drifting closer with a radial velocity of −5 km/s.[1]
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Mensa |
Right ascension | 04h 58m 50.96791s[1] |
Declination | −82° 28′ 13.8521″[1] |
Apparent magnitude (V) | 5.84[2] |
Characteristics | |
Spectral type | G8/K0III[3] |
B−V color index | 0.932±0.006[2] |
Astrometry | |
Radial velocity (Rv) | −4.7±0.2[1] km/s |
Proper motion (μ) | RA: −4.701±0.091[1] mas/yr Dec.: +2.648±0.107[1] mas/yr |
Parallax (π) | 9.6939 ± 0.0535 mas[1] |
Distance | 336 ± 2 ly (103.2 ± 0.6 pc) |
Absolute magnitude (MV) | 0.57[2] |
Details | |
Mass | 1.91[4] M☉ |
Radius | 8.97+0.22 −0.55[1] R☉ |
Luminosity | 50.3±0.4[1] L☉ |
Surface gravity (log g) | 3.02[5] cgs |
Temperature | 5,131+166 −60[1] K |
Metallicity [Fe/H] | 0.06[5] dex |
Age | 281[4] Myr |
Other designations | |
Database references | |
SIMBAD | data |
This object is an aging giant star with a stellar classification of G8/K0III.[3] It is 281[4] million years old with 1.91[4] times the mass of the Sun. The star displays micro-variability, fluctuating in brightness by 0.0049 magnitudes with a period of 148 days.[8] With the supply of hydrogen at its core exhausted, the star has cooled and expanded to nine[1] times the Sun's radius. It is radiating 50 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 5,131 K.[1]