Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Apus |
Right ascension | 14h 08m 27.1634s[1] |
Declination | −74° 51′ 01.0329″[1] |
Apparent magnitude (V) | 6.02[2] |
Characteristics | |
Spectral type | G2/3 IV[3] |
U−B color index | +0.06[4] |
B−V color index | +0.58[4] |
Astrometry | |
Radial velocity (Rv) | −21.11±0.16[5] km/s |
Proper motion (μ) | RA: −243.574[1] mas/yr Dec.: +179.540[1] mas/yr |
Parallax (π) | 34.1491 ± 0.0256 mas[1] |
Distance | 95.51 ± 0.07 ly (29.28 ± 0.02 pc) |
Absolute magnitude (MV) | +3.75[2] |
Details[6] | |
Mass | 1.08+0.02 −0.01 M☉ |
Radius | 1.58+0.03 −0.05[5] R☉ |
Luminosity | 2.87±0.01[5] L☉ |
Surface gravity (log g) | 4.10±0.03 cgs |
Temperature | 5,943±50 K |
Metallicity [Fe/H] | −0.15±0.04 dex |
Rotational velocity (v sin i) | 3.1±1[7] km/s |
Age | 6.83+0.39 −0.57 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 122862 (HR 5279) is a solitary star in the southern circumpolar constellation Apus. It has an apparent magnitude of 6.02,[2] allowing it to be faintly seen with the naked eye under ideal conditions. The star is relatively close at a distance of 95 light years,[1] but is approaching the Sun with a radial velocity of −21.11 km/s.[5]
HD 122862 is a G-type subgiant[3] with 1.08 times the mass of the Sun[6] and a diameter of 1.58 R☉.[5] It shines at 2.87 times the luminosity of the Sun[5] from its photosphere at an effective temperature of 5,943 K,[6] giving it a yellow glow. HD 122862 has an iron abundance 71% that of the Sun[6] and, at an age of 6.83 billion years,[6] it spins slowly with a projected rotational velocity of 3.1 km/s.[7]
EDR3
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Houk1975
was invoked but never defined (see the help page).Johnson1966
was invoked but never defined (see the help page).DR2
was invoked but never defined (see the help page).A.G2018
was invoked but never defined (see the help page).DeMederios2014
was invoked but never defined (see the help page).